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j		 dRd,d-Ze
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j		 	dWdJdKZ*dS )X    )IterableN)normalize_axis_index   )_ni_support)	_nd_image)_ni_docstrings)correlate1d
convolve1dgaussian_filter1dgaussian_filterprewittsobelgeneric_laplacelaplacegaussian_laplacegeneric_gradient_magnitudegaussian_gradient_magnitude	correlateconvolveuniform_filter1duniform_filterminimum_filter1dmaximum_filter1dminimum_filtermaximum_filterrank_filtermedian_filterpercentile_filtergeneric_filter1dgeneric_filterc                 C   s   | |d  k p| |d d kS )N   r    )originlenwr!   r!   =/tmp/pip-target-vg8gfxp4/lib/python/scipy/ndimage/_filters.py_invalid_origin2   s   r%   c                 K   s^  |j jdk}|j jdk}|rb|rb| |j|jf|jt|d| | j| |j|jfdt|d|8  _| |j|jf|jt|d| | j| |j|jfdt|d|7  _|S |r| |j|f|jt|d| | |j|f|jt|d| |S t|rtd| ||jf|j|d| | ||jf|j|d| |S )zBComplex convolution via a linear combination of real convolutions.c)outputcvalNz<Cannot provide a complex-valued cval when the input is real.)dtypekindrealnumpyimagiscomplexobj
ValueError)funcinputweightsr'   r(   kwargscomplex_inputcomplex_weightsr!   r!   r$   _complex_via_real_components6   sJ   


r6   reflect        c           
   	   C   s  t | } t |}| jjdk}|jjdk}|s|rC|r(| }|jt jdd}t|||d}	tj	|| dd}t
t| |||fi |	S t	|| }t j|t jd}|jdks]|jd	 dk ratd
|jjsi| }t|| j}t|t|rztdt|}t| |||||| |S )a  Calculate a 1-D correlation along the given axis.

    The lines of the array along the given axis are correlated with the
    given weights.

    Parameters
    ----------
    %(input)s
    weights : array
        1-D sequence of numbers.
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s

    Examples
    --------
    >>> from scipy.ndimage import correlate1d
    >>> correlate1d([2, 8, 0, 4, 1, 9, 9, 0], weights=[1, 3])
    array([ 8, 26,  8, 12,  7, 28, 36,  9])
    r&   F)copy)axismoder"   Tcomplex_outputr)   r   r   zno filter weights givenz[Invalid origin; origin must satisfy -(len(weights) // 2) <= origin <= (len(weights)-1) // 2)r,   asarrayr)   r*   conjastype
complex128dictr   _get_outputr6   r   float64ndimshapeRuntimeErrorflags
contiguousr:   r   r%   lenr/   _extend_mode_to_coder   )
r1   r2   r;   r'   r<   r(   r"   r4   r5   r3   r!   r!   r$   r   S   s:   


r   c                 C   sZ   |ddd }| }t |d@ s|d8 }t|}|jjdkr#| }t| ||||||S )aV  Calculate a 1-D convolution along the given axis.

    The lines of the array along the given axis are convolved with the
    given weights.

    Parameters
    ----------
    %(input)s
    weights : ndarray
        1-D sequence of numbers.
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s

    Returns
    -------
    convolve1d : ndarray
        Convolved array with same shape as input

    Examples
    --------
    >>> from scipy.ndimage import convolve1d
    >>> convolve1d([2, 8, 0, 4, 1, 9, 9, 0], weights=[1, 3])
    array([14, 24,  4, 13, 12, 36, 27,  0])
    Nr7   r   r&   )rL   r,   r@   r)   r*   rA   r   )r1   r2   r;   r'   r<   r(   r"   r!   r!   r$   r	      s   
r	   c                 C   s   |dk rt dt|d }| |  }t| |d }td| |d  }||  }|dkr3|S t|d }d|d< t|dd d}tt||  d}	||	 }
t|D ]}|
	|}q\|dddf | 	|}|| S )z5
    Computes a 1-D Gaussian convolution kernel.
    r   zorder must be non-negativer   g      r    Nr7   )
r/   r,   arangeexpsumzerosdiagonesrangedot)sigmaorderradiusexponent_rangesigma2xphi_xqDPQ_deriv_r!   r!   r$   _gaussian_kernel1d   s$   rb         @c                 C   sB   t |}t|| d }	t|||	ddd }
t| |
||||dS )a-  1-D Gaussian filter.

    Parameters
    ----------
    %(input)s
    sigma : scalar
        standard deviation for Gaussian kernel
    %(axis)s
    order : int, optional
        An order of 0 corresponds to convolution with a Gaussian
        kernel. A positive order corresponds to convolution with
        that derivative of a Gaussian.
    %(output)s
    %(mode_reflect)s
    %(cval)s
    truncate : float, optional
        Truncate the filter at this many standard deviations.
        Default is 4.0.

    Returns
    -------
    gaussian_filter1d : ndarray

    Examples
    --------
    >>> from scipy.ndimage import gaussian_filter1d
    >>> gaussian_filter1d([1.0, 2.0, 3.0, 4.0, 5.0], 1)
    array([ 1.42704095,  2.06782203,  3.        ,  3.93217797,  4.57295905])
    >>> gaussian_filter1d([1.0, 2.0, 3.0, 4.0, 5.0], 4)
    array([ 2.91948343,  2.95023502,  3.        ,  3.04976498,  3.08051657])
    >>> import matplotlib.pyplot as plt
    >>> rng = np.random.default_rng()
    >>> x = rng.standard_normal(101).cumsum()
    >>> y3 = gaussian_filter1d(x, 3)
    >>> y6 = gaussian_filter1d(x, 6)
    >>> plt.plot(x, 'k', label='original data')
    >>> plt.plot(y3, '--', label='filtered, sigma=3')
    >>> plt.plot(y6, ':', label='filtered, sigma=6')
    >>> plt.legend()
    >>> plt.grid()
    >>> plt.show()

    g      ?Nr7   r   )floatintrb   r   )r1   rV   r;   rW   r'   r<   r(   truncatesdlwr2   r!   r!   r$   r
      s   .r
   c              
      s   t | } t|| }t|| jt|| jt|| jtt| j  fddtt D  t dkrU D ]\}}}}t	| ||||||| |} q?|S | d |d< |S )a  Multidimensional Gaussian filter.

    Parameters
    ----------
    %(input)s
    sigma : scalar or sequence of scalars
        Standard deviation for Gaussian kernel. The standard
        deviations of the Gaussian filter are given for each axis as a
        sequence, or as a single number, in which case it is equal for
        all axes.
    order : int or sequence of ints, optional
        The order of the filter along each axis is given as a sequence
        of integers, or as a single number. An order of 0 corresponds
        to convolution with a Gaussian kernel. A positive order
        corresponds to convolution with that derivative of a Gaussian.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    truncate : float
        Truncate the filter at this many standard deviations.
        Default is 4.0.

    Returns
    -------
    gaussian_filter : ndarray
        Returned array of same shape as `input`.

    Notes
    -----
    The multidimensional filter is implemented as a sequence of
    1-D convolution filters. The intermediate arrays are
    stored in the same data type as the output. Therefore, for output
    types with a limited precision, the results may be imprecise
    because intermediate results may be stored with insufficient
    precision.

    Examples
    --------
    >>> from scipy.ndimage import gaussian_filter
    >>> a = np.arange(50, step=2).reshape((5,5))
    >>> a
    array([[ 0,  2,  4,  6,  8],
           [10, 12, 14, 16, 18],
           [20, 22, 24, 26, 28],
           [30, 32, 34, 36, 38],
           [40, 42, 44, 46, 48]])
    >>> gaussian_filter(a, sigma=1)
    array([[ 4,  6,  8,  9, 11],
           [10, 12, 14, 15, 17],
           [20, 22, 24, 25, 27],
           [29, 31, 33, 34, 36],
           [35, 37, 39, 40, 42]])

    >>> from scipy import misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = gaussian_filter(ascent, sigma=5)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    c                    4   g | ]}| d kr | | | | fqS )gV瞯<r!   .0iiaxesmodesorderssigmasr!   r$   
<listcomp>R      "z#gaussian_filter.<locals>.<listcomp>r   .)
r,   r@   r   rE   _normalize_sequencerG   listrT   rL   r
   )r1   rV   rW   r'   r<   r(   rf   r;   r!   rm   r$   r     s$   
D
r   c              	         t | } t | j t|| }t|| j}t| g d ||  |d  fddt| jD }|D ]}t|g d|||| |d q4|S )a@  Calculate a Prewitt filter.

    Parameters
    ----------
    %(input)s
    %(axis)s
    %(output)s
    %(mode_multiple)s
    %(cval)s

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.prewitt(ascent)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    r7   r   r   r   c                       g | ]}| kr|qS r!   r!   rj   r;   r!   r$   rr   }      zprewitt.<locals>.<listcomp>)r   r   r   	r,   r@   r   rG   r   rE   rt   r   rT   r1   r;   r'   r<   r(   ro   rn   rl   r!   ry   r$   r   ^     
r   c              	      rv   )a<  Calculate a Sobel filter.

    Parameters
    ----------
    %(input)s
    %(axis)s
    %(output)s
    %(mode_multiple)s
    %(cval)s

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.sobel(ascent)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    rw   r   c                    rx   r!   r!   rj   ry   r!   r$   rr     rz   zsobel.<locals>.<listcomp>)r   r    r   r{   r|   r!   ry   r$   r     r}   r   r!   c                 C   s   |du ri }t | } t|| }tt| j}t|dkr]t|t|}|| |d ||d |g|R i | tdt|D ]}	|| ||	 |j	||	 |g|R i |}
||
7 }q@|S | d |d< |S )a  
    N-D Laplace filter using a provided second derivative function.

    Parameters
    ----------
    %(input)s
    derivative2 : callable
        Callable with the following signature::

            derivative2(input, axis, output, mode, cval,
                        *extra_arguments, **extra_keywords)

        See `extra_arguments`, `extra_keywords` below.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    %(extra_keywords)s
    %(extra_arguments)s
    Nr   r   .)
r,   r@   r   rE   ru   rT   rG   rL   rt   r)   )r1   derivative2r'   r<   r(   extra_argumentsextra_keywordsrn   ro   rl   tmpr!   r!   r$   r     s,   

r   c                 C   s   dd }t | ||||S )aS  N-D Laplace filter based on approximate second derivatives.

    Parameters
    ----------
    %(input)s
    %(output)s
    %(mode_multiple)s
    %(cval)s

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.laplace(ascent)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    c                 S   s   t | g d||||dS )N)r   r   r   )r   )r1   r;   r'   r<   r(   r!   r!   r$   r~     s   zlaplace.<locals>.derivative2)r   )r1   r'   r<   r(   r~   r!   r!   r$   r     s   r   c              	   K   *   t | } dd }t| |||||f|dS )a  Multidimensional Laplace filter using Gaussian second derivatives.

    Parameters
    ----------
    %(input)s
    sigma : scalar or sequence of scalars
        The standard deviations of the Gaussian filter are given for
        each axis as a sequence, or as a single number, in which case
        it is equal for all axes.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    Extra keyword arguments will be passed to gaussian_filter().

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> ascent = misc.ascent()

    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side

    >>> result = ndimage.gaussian_laplace(ascent, sigma=1)
    >>> ax1.imshow(result)

    >>> result = ndimage.gaussian_laplace(ascent, sigma=3)
    >>> ax2.imshow(result)
    >>> plt.show()
    c                 [   .   dg| j  }d||< t| |||||fi |S )Nr   r    rG   r   r1   r;   r'   r<   r(   rV   r3   rW   r!   r!   r$   r~     s
   z%gaussian_laplace.<locals>.derivative2r   r   )r,   r@   r   )r1   rV   r'   r<   r(   r3   r~   r!   r!   r$   r     s   
#r   c                 C   s   |du ri }t | } t|| }tt| j}t|dkrst|t|}|| |d ||d |g|R i | t 	||| tdt|D ]!}	|| ||	 |j
||	 |g|R i |}
t 	|
|
|
 ||
7 }qGt j||dd |S | d |d< |S )a  Gradient magnitude using a provided gradient function.

    Parameters
    ----------
    %(input)s
    derivative : callable
        Callable with the following signature::

            derivative(input, axis, output, mode, cval,
                       *extra_arguments, **extra_keywords)

        See `extra_arguments`, `extra_keywords` below.
        `derivative` can assume that `input` and `output` are ndarrays.
        Note that the output from `derivative` is modified inplace;
        be careful to copy important inputs before returning them.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    %(extra_keywords)s
    %(extra_arguments)s
    Nr   r   unsafe)casting.)r,   r@   r   rE   ru   rT   rG   rL   rt   multiplyr)   sqrt)r1   
derivativer'   r<   r(   r   r   rn   ro   rl   r   r!   r!   r$   r      s2   

r   c              	   K   r   )a  Multidimensional gradient magnitude using Gaussian derivatives.

    Parameters
    ----------
    %(input)s
    sigma : scalar or sequence of scalars
        The standard deviations of the Gaussian filter are given for
        each axis as a sequence, or as a single number, in which case
        it is equal for all axes.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    Extra keyword arguments will be passed to gaussian_filter().

    Returns
    -------
    gaussian_gradient_magnitude : ndarray
        Filtered array. Has the same shape as `input`.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.gaussian_gradient_magnitude(ascent, sigma=5)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    c                 [   r   )Nr   r   r   r   r!   r!   r$   r   u  s   z/gaussian_gradient_magnitude.<locals>.derivativer   )r,   r@   r   )r1   rV   r'   r<   r(   r3   r   r!   r!   r$   r   O  s   
$
r   c                 C   s  t | } t |}| jjdk}|jjdk}|s|r=|r"|s"| }t|||d}	tj|| dd}tt	| |||fi |	S t
|| j}
t j|t jd}dd |jD }t|| jkr_td|r|ttd d d	g|j  }tt|
D ]}|
|  |
|< |j| d
@ s|
|  d
8  < qut|
|D ]\}}t||rtdq|jjs| }t|| }t | |}|r|}t|j| }t|tst|trtdt|}t| |||||
 |r||d< |}|S )Nr&   )r<   r"   convolutionTr=   r?   c                 S      g | ]}|d kr|qS r   r!   rj   r!   r!   r$   rr     rz   z*_correlate_or_convolve.<locals>.<listcomp>z)filter weights array has incorrect shape.r7   r   zfInvalid origin; origin must satisfy -(weights.shape[k] // 2) <= origin[k] <= (weights.shape[k]-1) // 2z$A sequence of modes is not supported.) r,   r@   r)   r*   rA   rD   r   rE   r6   _correlate_or_convolvert   rG   rF   rH   rL   rI   tupleslicerT   zipr%   r/   rJ   rK   r:   may_share_memory
isinstancestrr   rM   r   r   )r1   r2   r'   r<   r(   r"   r   r4   r5   r3   originswshaperl   r#   temp_neededtempr!   r!   r$   r     s^   



r   c                 C      t | |||||dS )a  
    Multidimensional correlation.

    The array is correlated with the given kernel.

    Parameters
    ----------
    %(input)s
    weights : ndarray
        array of weights, same number of dimensions as input
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    result : ndarray
        The result of correlation of `input` with `weights`.

    See Also
    --------
    convolve : Convolve an image with a kernel.

    Examples
    --------
    Correlation is the process of moving a filter mask often referred to
    as kernel over the image and computing the sum of products at each location.

    >>> from scipy.ndimage import correlate
    >>> input_img = np.arange(25).reshape(5,5)
    >>> print(input_img)
    [[ 0  1  2  3  4]
    [ 5  6  7  8  9]
    [10 11 12 13 14]
    [15 16 17 18 19]
    [20 21 22 23 24]]

    Define a kernel (weights) for correlation. In this example, it is for sum of
    center and up, down, left and right next elements.

    >>> weights = [[0, 1, 0],
    ...            [1, 1, 1],
    ...            [0, 1, 0]]

    We can calculate a correlation result:
    For example, element ``[2,2]`` is ``7 + 11 + 12 + 13 + 17 = 60``.

    >>> correlate(input_img, weights)
    array([[  6,  10,  15,  20,  24],
        [ 26,  30,  35,  40,  44],
        [ 51,  55,  60,  65,  69],
        [ 76,  80,  85,  90,  94],
        [ 96, 100, 105, 110, 114]])

    Fr   r1   r2   r'   r<   r(   r"   r!   r!   r$   r     s   ;r   c                 C   r   )a  
    Multidimensional convolution.

    The array is convolved with the given kernel.

    Parameters
    ----------
    %(input)s
    weights : array_like
        Array of weights, same number of dimensions as input
    %(output)s
    %(mode_reflect)s
    cval : scalar, optional
        Value to fill past edges of input if `mode` is 'constant'. Default
        is 0.0
    origin : int, optional
        Controls the origin of the input signal, which is where the
        filter is centered to produce the first element of the output.
        Positive values shift the filter to the right, and negative values
        shift the filter to the left. Default is 0.

    Returns
    -------
    result : ndarray
        The result of convolution of `input` with `weights`.

    See Also
    --------
    correlate : Correlate an image with a kernel.

    Notes
    -----
    Each value in result is :math:`C_i = \sum_j{I_{i+k-j} W_j}`, where
    W is the `weights` kernel,
    j is the N-D spatial index over :math:`W`,
    I is the `input` and k is the coordinate of the center of
    W, specified by `origin` in the input parameters.

    Examples
    --------
    Perhaps the simplest case to understand is ``mode='constant', cval=0.0``,
    because in this case borders (i.e., where the `weights` kernel, centered
    on any one value, extends beyond an edge of `input`) are treated as zeros.

    >>> a = np.array([[1, 2, 0, 0],
    ...               [5, 3, 0, 4],
    ...               [0, 0, 0, 7],
    ...               [9, 3, 0, 0]])
    >>> k = np.array([[1,1,1],[1,1,0],[1,0,0]])
    >>> from scipy import ndimage
    >>> ndimage.convolve(a, k, mode='constant', cval=0.0)
    array([[11, 10,  7,  4],
           [10,  3, 11, 11],
           [15, 12, 14,  7],
           [12,  3,  7,  0]])

    Setting ``cval=1.0`` is equivalent to padding the outer edge of `input`
    with 1.0's (and then extracting only the original region of the result).

    >>> ndimage.convolve(a, k, mode='constant', cval=1.0)
    array([[13, 11,  8,  7],
           [11,  3, 11, 14],
           [16, 12, 14, 10],
           [15,  6, 10,  5]])

    With ``mode='reflect'`` (the default), outer values are reflected at the
    edge of `input` to fill in missing values.

    >>> b = np.array([[2, 0, 0],
    ...               [1, 0, 0],
    ...               [0, 0, 0]])
    >>> k = np.array([[0,1,0], [0,1,0], [0,1,0]])
    >>> ndimage.convolve(b, k, mode='reflect')
    array([[5, 0, 0],
           [3, 0, 0],
           [1, 0, 0]])

    This includes diagonally at the corners.

    >>> k = np.array([[1,0,0],[0,1,0],[0,0,1]])
    >>> ndimage.convolve(b, k)
    array([[4, 2, 0],
           [3, 2, 0],
           [1, 1, 0]])

    With ``mode='nearest'``, the single nearest value in to an edge in
    `input` is repeated as many times as needed to match the overlapping
    `weights`.

    >>> c = np.array([[2, 0, 1],
    ...               [1, 0, 0],
    ...               [0, 0, 0]])
    >>> k = np.array([[0, 1, 0],
    ...               [0, 1, 0],
    ...               [0, 1, 0],
    ...               [0, 1, 0],
    ...               [0, 1, 0]])
    >>> ndimage.convolve(c, k, mode='nearest')
    array([[7, 0, 3],
           [5, 0, 2],
           [3, 0, 1]])

    Tr   r   r!   r!   r$   r     s   jr   c              
   C   s   t | } t|| j}|dk rtd| jjdk}tj|| |d}|d | dk s1|d | |kr5t	dt
|}|sIt| |||||| |S t| j|||j|t || t| j|||j|t || |S )a  Calculate a 1-D uniform filter along the given axis.

    The lines of the array along the given axis are filtered with a
    uniform filter of given size.

    Parameters
    ----------
    %(input)s
    size : int
        length of uniform filter
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s

    Examples
    --------
    >>> from scipy.ndimage import uniform_filter1d
    >>> uniform_filter1d([2, 8, 0, 4, 1, 9, 9, 0], size=3)
    array([4, 3, 4, 1, 4, 6, 6, 3])
    r   incorrect filter sizer&   r=   r    r   invalid origin)r,   r@   r   rG   rI   r)   r*   r   rE   r/   rM   r   r   r+   r-   )r1   sizer;   r'   r<   r(   r"   r>   r!   r!   r$   r   b  s.   
 


r      c              	      s   t | } tj|| | jjdkd}t|| jt|| jt|| jtt	| j  fddt	t
 D  t
 dkr\ D ]\}}}}t| t|||||| |} qE|S | d |d< |S )a  Multidimensional uniform filter.

    Parameters
    ----------
    %(input)s
    size : int or sequence of ints, optional
        The sizes of the uniform filter are given for each axis as a
        sequence, or as a single number, in which case the size is
        equal for all axes.
    %(output)s
    %(mode_multiple)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    uniform_filter : ndarray
        Filtered array. Has the same shape as `input`.

    Notes
    -----
    The multidimensional filter is implemented as a sequence of
    1-D uniform filters. The intermediate arrays are stored
    in the same data type as the output. Therefore, for output types
    with a limited precision, the results may be imprecise because
    intermediate results may be stored with insufficient precision.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.uniform_filter(ascent, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    r&   r=   c                    ri   r   r!   rj   rn   ro   r   sizesr!   r$   rr     rs   z"uniform_filter.<locals>.<listcomp>r   .)r,   r@   r   rE   r)   r*   rt   rG   ru   rT   rL   r   re   )r1   r   r'   r<   r(   r"   r;   r!   r   r$   r     s(   
,

r   c              
   C   s   t | } t | rtdt|| j}|dk rtdt|| }|d | dk s2|d | |kr6t	dt
|}t| ||||||d |S )a  Calculate a 1-D minimum filter along the given axis.

    The lines of the array along the given axis are filtered with a
    minimum filter of given size.

    Parameters
    ----------
    %(input)s
    size : int
        length along which to calculate 1D minimum
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s

    Notes
    -----
    This function implements the MINLIST algorithm [1]_, as described by
    Richard Harter [2]_, and has a guaranteed O(n) performance, `n` being
    the `input` length, regardless of filter size.

    References
    ----------
    .. [1] http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.42.2777
    .. [2] http://www.richardhartersworld.com/cri/2001/slidingmin.html


    Examples
    --------
    >>> from scipy.ndimage import minimum_filter1d
    >>> minimum_filter1d([2, 8, 0, 4, 1, 9, 9, 0], size=3)
    array([2, 0, 0, 0, 1, 1, 0, 0])
    Complex type not supportedr   r   r    r   r   r,   r@   r.   	TypeErrorr   rG   rI   r   rE   r/   rM   r   min_or_max_filter1dr1   r   r;   r'   r<   r(   r"   r!   r!   r$   r     s   
%
 
r   c              
   C   s   t | } t | rtdt|| j}|dk rtdt|| }|d | dk s2|d | |kr6t	dt
|}t| ||||||d |S )a0  Calculate a 1-D maximum filter along the given axis.

    The lines of the array along the given axis are filtered with a
    maximum filter of given size.

    Parameters
    ----------
    %(input)s
    size : int
        Length along which to calculate the 1-D maximum.
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s

    Returns
    -------
    maximum1d : ndarray, None
        Maximum-filtered array with same shape as input.
        None if `output` is not None

    Notes
    -----
    This function implements the MAXLIST algorithm [1]_, as described by
    Richard Harter [2]_, and has a guaranteed O(n) performance, `n` being
    the `input` length, regardless of filter size.

    References
    ----------
    .. [1] http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.42.2777
    .. [2] http://www.richardhartersworld.com/cri/2001/slidingmin.html

    Examples
    --------
    >>> from scipy.ndimage import maximum_filter1d
    >>> maximum_filter1d([2, 8, 0, 4, 1, 9, 9, 0], size=3)
    array([8, 8, 8, 4, 9, 9, 9, 9])
    r   r   r   r    r   r   r   r   r!   r!   r$   r     s   
*
 
r   c	              
      s  |d ur|d urt jdtdd |d u rA|d u r#|d u r tdd}	n;tj|td}| s2td|	 r>|j
}d }d}	n d}	ntj|tjd}d}	|d u rWt|j
t}ntj|td}t| } t| rltd	t|| }t| |}
|
r|}t|j| }t|| j|	rt|| jt|| jtt| j  fd
dtt D  |rt}nt}t dkrֈ D ]\}}}}|| t|||||| |} qn| d |d< nxdd |j
D }t|| jkrtdt|D ]\}}|d | dk s|d | |krtdq|jjs| }|d ur4t|j
| jkr+td|jjs4| }t|t sDt|t!rDtdt"|}t#$| |||||| |
r^||d< |}|S )N&ignoring size because footprint is setr   
stacklevelzno footprint providedTr?   z$All-zero footprint is not supported.Fr   c                    ri   r   r!   rj   r   r!   r$   rr   d  rs   z&_min_or_max_filter.<locals>.<listcomp>r   .c                 S   r   r   r!   rj   r!   r!   r$   rr   q  rz   z$footprint array has incorrect shape.r    r   z#structure array has incorrect shapezAA sequence of modes is not supported for non-separable footprints)%warningswarnUserWarningrI   r,   r@   boolanyr/   allrH   rF   rS   r.   r   r   rE   r   r)   rt   rG   ru   rT   rL   r   r   re   r   rJ   rK   r:   r   r   r   rM   r   min_or_max_filter)r1   r   	footprint	structurer'   r<   r(   r"   minimum	separabler   r   filter_r;   fshapelenfr!   r   r$   _min_or_max_filter<  s   


$



r   c              
   C      t | ||d||||d	S )a  Calculate a multidimensional minimum filter.

    Parameters
    ----------
    %(input)s
    %(size_foot)s
    %(output)s
    %(mode_multiple)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    minimum_filter : ndarray
        Filtered array. Has the same shape as `input`.

    Notes
    -----
    A sequence of modes (one per axis) is only supported when the footprint is
    separable. Otherwise, a single mode string must be provided.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.minimum_filter(ascent, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    Nr   r   r1   r   r   r'   r<   r(   r"   r!   r!   r$   r        &r   c              
   C   r   )a  Calculate a multidimensional maximum filter.

    Parameters
    ----------
    %(input)s
    %(size_foot)s
    %(output)s
    %(mode_multiple)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    maximum_filter : ndarray
        Filtered array. Has the same shape as `input`.

    Notes
    -----
    A sequence of modes (one per axis) is only supported when the footprint is
    separable. Otherwise, a single mode string must be provided.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.maximum_filter(ascent, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    Nr   r   r   r!   r!   r$   r     r   r   rankc	              	   C   sh  |d ur|d urt jdtdd t| } t| rtdt|| j	}	|d u r@|d u r1t
dt|| j	}
tj|
td}ntj|td}dd |jD }t|| j	krZt
d	t|	|D ]\}}|d
 | dk ss|d
 | |krwtdq_|jjs| }t|dd }|dkr|d
 }n-|dkr|}|dk r|d7 }|dk s|dkrt
d|dkr|d }n
tt|| d }|dk r||7 }|dk s||krt
d|dkrt| d |||||	S ||d krt| d |||||	S t|| }t| |}|r	|}t|j| }t|tst|trt
dt |}t!"| ||||||	 |r2||d< |}|S )Nr   r   r   r   $no footprint or filter size providedr?   c                 S   r   r   r!   rj   r!   r!   r$   rr     rz   z _rank_filter.<locals>.<listcomp>+filter footprint array has incorrect shape.r    r   r   r   median
percentiler9   g      Y@d   zinvalid percentilez%rank not within filter footprint sizezBA sequence of modes is not supported by non-separable rank filters.)#r   r   r   r,   r@   r.   r   r   rt   rG   rI   rS   r   rH   rL   r   r/   rJ   rK   r:   whererP   re   rd   r   r   rE   r   r)   r   r   r   rM   r   r   )r1   r   r   r   r'   r<   r(   r"   	operationr   r   r   r   filter_sizer   r   r   r!   r!   r$   _rank_filter  s|   

 


r   c              
   C   s"   t |}t| |||||||d	S )ab  Calculate a multidimensional rank filter.

    Parameters
    ----------
    %(input)s
    rank : int
        The rank parameter may be less than zero, i.e., rank = -1
        indicates the largest element.
    %(size_foot)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    rank_filter : ndarray
        Filtered array. Has the same shape as `input`.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.rank_filter(ascent, rank=42, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    r   )operatorindexr   )r1   r   r   r   r'   r<   r(   r"   r!   r!   r$   r   "  s   
$r   c              
   C   s   t | d||||||d	S )a  
    Calculate a multidimensional median filter.

    Parameters
    ----------
    %(input)s
    %(size_foot)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    median_filter : ndarray
        Filtered array. Has the same shape as `input`.

    See Also
    --------
    scipy.signal.medfilt2d

    Notes
    -----
    For 2-dimensional images with ``uint8``, ``float32`` or ``float64`` dtypes
    the specialised function `scipy.signal.medfilt2d` may be faster. It is
    however limited to constant mode with ``cval=0``.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.median_filter(ascent, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    r   r   r   r   r!   r!   r$   r   K  s   ,r   c              
   C   s   t | |||||||d	S )a  Calculate a multidimensional percentile filter.

    Parameters
    ----------
    %(input)s
    percentile : scalar
        The percentile parameter may be less than zero, i.e.,
        percentile = -20 equals percentile = 80
    %(size_foot)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin_multiple)s

    Returns
    -------
    percentile_filter : ndarray
        Filtered array. Has the same shape as `input`.

    Examples
    --------
    >>> from scipy import ndimage, misc
    >>> import matplotlib.pyplot as plt
    >>> fig = plt.figure()
    >>> plt.gray()  # show the filtered result in grayscale
    >>> ax1 = fig.add_subplot(121)  # left side
    >>> ax2 = fig.add_subplot(122)  # right side
    >>> ascent = misc.ascent()
    >>> result = ndimage.percentile_filter(ascent, percentile=20, size=20)
    >>> ax1.imshow(ascent)
    >>> ax2.imshow(result)
    >>> plt.show()
    r   r   )r1   r   r   r   r'   r<   r(   r"   r!   r!   r$   r   {  s   $r   c
           
      C   s   |	du ri }	t | } t | rtdt|| }|dk r"tdt|| j}|d | dk s8|d | |kr<t	dt
|}t| |||||||||	
 |S )ax	  Calculate a 1-D filter along the given axis.

    `generic_filter1d` iterates over the lines of the array, calling the
    given function at each line. The arguments of the line are the
    input line, and the output line. The input and output lines are 1-D
    double arrays. The input line is extended appropriately according
    to the filter size and origin. The output line must be modified
    in-place with the result.

    Parameters
    ----------
    %(input)s
    function : {callable, scipy.LowLevelCallable}
        Function to apply along given axis.
    filter_size : scalar
        Length of the filter.
    %(axis)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin)s
    %(extra_arguments)s
    %(extra_keywords)s

    Notes
    -----
    This function also accepts low-level callback functions with one of
    the following signatures and wrapped in `scipy.LowLevelCallable`:

    .. code:: c

       int function(double *input_line, npy_intp input_length,
                    double *output_line, npy_intp output_length,
                    void *user_data)
       int function(double *input_line, intptr_t input_length,
                    double *output_line, intptr_t output_length,
                    void *user_data)

    The calling function iterates over the lines of the input and output
    arrays, calling the callback function at each line. The current line
    is extended according to the border conditions set by the calling
    function, and the result is copied into the array that is passed
    through ``input_line``. The length of the input line (after extension)
    is passed through ``input_length``. The callback function should apply
    the filter and store the result in the array passed through
    ``output_line``. The length of the output line is passed through
    ``output_length``. ``user_data`` is the data pointer provided
    to `scipy.LowLevelCallable` as-is.

    The callback function must return an integer error status that is zero
    if something went wrong and one otherwise. If an error occurs, you should
    normally set the python error status with an informative message
    before returning, otherwise a default error message is set by the
    calling function.

    In addition, some other low-level function pointer specifications
    are accepted, but these are for backward compatibility only and should
    not be used in new code.

    Nr   r   zinvalid filter sizer    r   r   )r,   r@   r.   r   r   rE   rI   r   rG   r/   rM   r   r   )
r1   functionr   r;   r'   r<   r(   r"   r   r   r!   r!   r$   r     s&   @


r   c
                 C   s@  |dur|durt jdtdd |	du ri }	t| } t| r$tdt|| j	}
|du rF|du r7t
dt|| j	}tj|td}ntj|td}dd	 |jD }t|| j	kr`t
d
t|
|D ]\}}|d | dk sy|d | |kr}tdqe|jjs| }t|| }t|}t| ||||||
||		 |S )at  Calculate a multidimensional filter using the given function.

    At each element the provided function is called. The input values
    within the filter footprint at that element are passed to the function
    as a 1-D array of double values.

    Parameters
    ----------
    %(input)s
    function : {callable, scipy.LowLevelCallable}
        Function to apply at each element.
    %(size_foot)s
    %(output)s
    %(mode_reflect)s
    %(cval)s
    %(origin_multiple)s
    %(extra_arguments)s
    %(extra_keywords)s

    Notes
    -----
    This function also accepts low-level callback functions with one of
    the following signatures and wrapped in `scipy.LowLevelCallable`:

    .. code:: c

       int callback(double *buffer, npy_intp filter_size,
                    double *return_value, void *user_data)
       int callback(double *buffer, intptr_t filter_size,
                    double *return_value, void *user_data)

    The calling function iterates over the elements of the input and
    output arrays, calling the callback function at each element. The
    elements within the footprint of the filter at the current element are
    passed through the ``buffer`` parameter, and the number of elements
    within the footprint through ``filter_size``. The calculated value is
    returned in ``return_value``. ``user_data`` is the data pointer provided
    to `scipy.LowLevelCallable` as-is.

    The callback function must return an integer error status that is zero
    if something went wrong and one otherwise. If an error occurs, you should
    normally set the python error status with an informative message
    before returning, otherwise a default error message is set by the
    calling function.

    In addition, some other low-level function pointer specifications
    are accepted, but these are for backward compatibility only and should
    not be used in new code.

    Nr   r    r   r   r   r?   c                 S   r   r   r!   rj   r!   r!   r$   rr   ;  rz   z"generic_filter.<locals>.<listcomp>r   r   r   )r   r   r   r,   r@   r.   r   r   rt   rG   rI   rS   r   rH   rL   r   r/   rJ   rK   r:   rE   rM   r   r   )r1   r   r   r   r'   r<   r(   r"   r   r   r   r   r   r   r!   r!   r$   r     s:   6

 
r   )r7   Nr8   r9   r   )r7   r   Nr8   r9   rc   )r   Nr8   r9   rc   )r7   Nr8   r9   )Nr8   r9   r!   N)Nr8   r9   )Nr8   r9   r   )r   Nr8   r9   r   )NNNr8   r9   r   )NNNr8   r9   r   r   )r7   Nr8   r9   r   r!   N)NNNr8   r9   r   r!   N)+collections.abcr   r   r,   r   numpy.core.multiarrayr    r   r   r   __all__r%   r6   	docfillerr   r	   rb   r
   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r   r!   r!   r!   r$   <module>   s   
6(5U$$)/.05>m->38O))B(/'R