colour.colorimetry.spectrum Module

Spectrum

Defines the classes handling spectral data computation:

See also

Spectrum IPython Notebook

class colour.colorimetry.spectrum.SpectralShape(start=None, end=None, steps=None)[source]

Bases: object

Defines the base object for spectral power distribution shape.

Parameters:
  • start (numeric, optional) – Wavelengths \(\lambda_{i}\): range start in nm.
  • end (numeric, optional) – Wavelengths \(\lambda_{i}\): range end in nm.
  • steps (numeric, optional) – Wavelengths \(\lambda_{i}\): range steps.
start[source]
end[source]
steps[source]
__repr__()[source]
__contains__()[source]
__len__()[source]
__eq__()[source]
__ne__()[source]
range()[source]

Examples

>>> SpectralShape(360, 830, 1)
SpectralShape(360, 830, 1)
__contains__(wavelength)[source]

Returns if the spectral shape contains the given wavelength \(\lambda\).

Parameters:wavelength (numeric) – Wavelength \(\lambda\).
Returns:Is wavelength \(\lambda\) in the spectral shape.
Return type:bool

Notes

  • Reimplements the object.__contains__() method.

Examples

>>> 0.5 in SpectralShape(0, 10, 0.1)
True
>>> 0.51 in SpectralShape(0, 10, 0.1)
False
__eq__(shape)[source]

Returns the spectral shape equality with given other spectral shape.

Parameters:shape (SpectralShape) – Spectral shape to compare for equality.
Returns:Spectral shape equality.
Return type:bool

Notes

  • Reimplements the object.__eq__() method.

Examples

>>> SpectralShape(0, 10, 0.1) == SpectralShape(0, 10, 0.1)
True
>>> SpectralShape(0, 10, 0.1) == SpectralShape(0, 10, 1)
False
__iter__()[source]

Returns a generator for the spectral power distribution data.

Returns:Spectral power distribution data generator.
Return type:generator

Notes

  • Reimplements the object.__iter__() method.

Examples

>>> shape = SpectralShape(0, 10, 1)
>>> for wavelength in shape: print(wavelength)
0
1
2
3
4
5
6
7
8
9
10
__len__()[source]

Returns the spectral shape wavelengths \(\lambda_n\) count.

Returns:Spectral shape wavelengths \(\lambda_n\) count.
Return type:int

Notes

  • Reimplements the object.__len__() method.

Examples

>>> len(SpectralShape(0, 10, 0.1))
101
__ne__(shape)[source]

Returns the spectral shape inequality with given other spectral shape.

Parameters:shape (SpectralShape) – Spectral shape to compare for inequality.
Returns:Spectral shape inequality.
Return type:bool

Notes

  • Reimplements the object.__ne__() method.

Examples

>>> SpectralShape(0, 10, 0.1) != SpectralShape(0, 10, 0.1)
False
>>> SpectralShape(0, 10, 0.1) != SpectralShape(0, 10, 1)
True
__repr__()[source]

Returns a formatted string representation.

Returns:Formatted string representation.
Return type:unicode
__str__()[source]

Returns a nice formatted string representation.

Returns:Nice formatted string representation.
Return type:unicode
end[source]

Property for self.__end private attribute.

Returns:self.__end.
Return type:numeric
range()[source]

Returns an iterable range for the spectral power distribution shape.

Returns:Iterable range for the spectral power distribution shape
Return type:ndarray
Raises:RuntimeError – If one of spectral shape start, end or steps attributes is not defined.

Examples

>>> SpectralShape(0, 10, 0.1).range()
array([  0. ,   0.1,   0.2,   0.3,   0.4,   0.5,   0.6,   0.7,   0.8,
         0.9,   1. ,   1.1,   1.2,   1.3,   1.4,   1.5,   1.6,   1.7,
         1.8,   1.9,   2. ,   2.1,   2.2,   2.3,   2.4,   2.5,   2.6,
         2.7,   2.8,   2.9,   3. ,   3.1,   3.2,   3.3,   3.4,   3.5,
         3.6,   3.7,   3.8,   3.9,   4. ,   4.1,   4.2,   4.3,   4.4,
         4.5,   4.6,   4.7,   4.8,   4.9,   5. ,   5.1,   5.2,   5.3,
         5.4,   5.5,   5.6,   5.7,   5.8,   5.9,   6. ,   6.1,   6.2,
         6.3,   6.4,   6.5,   6.6,   6.7,   6.8,   6.9,   7. ,   7.1,
         7.2,   7.3,   7.4,   7.5,   7.6,   7.7,   7.8,   7.9,   8. ,
         8.1,   8.2,   8.3,   8.4,   8.5,   8.6,   8.7,   8.8,   8.9,
         9. ,   9.1,   9.2,   9.3,   9.4,   9.5,   9.6,   9.7,   9.8,
         9.9,  10. ])
start[source]

Property for self.__start private attribute.

Returns:self.__start.
Return type:numeric
steps[source]

Property for self.__steps private attribute.

Returns:self.__steps.
Return type:numeric
class colour.colorimetry.spectrum.SpectralPowerDistribution(name, data)[source]

Bases: object

Defines the base object for spectral data computations.

Parameters:
  • name (str or unicode) – Spectral power distribution name.
  • data (dict) – Spectral power distribution data in a dict as follows: {wavelength \(\lambda_{i}\): value, wavelength \(\lambda_{i+1}\), ..., wavelength \(\lambda_{i+n}\)}
name[source]
data[source]
wavelengths[source]
values[source]
items[source]
shape[source]
__getitem__()[source]
__init__()[source]
__setitem__()[source]
__iter__()[source]
__contains__()[source]
__len__()[source]
__eq__()[source]
__ne__()[source]
__add__()[source]
__sub__()[source]
__mul__()[source]
__div__()[source]
__truediv__()
get()[source]
is_uniform()[source]
extrapolate()[source]
interpolate()[source]
align()[source]
zeros()[source]
normalise()[source]
clone()[source]

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.wavelengths
array([510, 520, 530, 540])
>>> spd.values
array([ 49.67,  69.59,  81.73,  88.19])
>>> spd.shape
SpectralShape(510, 540, 10)
__add__(x)[source]

Implements support for spectral power distribution addition.

Parameters:x (numeric or array_like or SpectralPowerDistribution) – Variable to add.
Returns:Variable added spectral power distribution.
Return type:SpectralPowerDistribution

See also

SpectralPowerDistribution.__sub__(), SpectralPowerDistribution.__mul__(), SpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__add__() method.

Warning

The addition operation happens in place.

Examples

Adding a single numeric variable:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd + 10  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 59.67,  79.59,  91.73,  98.19])

Adding an array_like variable:

>>> spd + [1, 2, 3, 4]  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([  60.67,   81.59,   94.73,  102.19])

Adding a SpectralPowerDistribution class variable:

>>> spd_alternate = SpectralPowerDistribution('Spd', data)
>>> spd + spd_alternate  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 110.34,  151.18,  176.46,  190.38])
__contains__(wavelength)[source]

Returns if the spectral power distribution contains the given wavelength \(\lambda\).

Parameters:wavelength (numeric) – Wavelength \(\lambda\).
Returns:Is wavelength \(\lambda\) in the spectral power distribution.
Return type:bool

Notes

  • Reimplements the object.__contains__() method.

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> 510 in spd
True
__div__(x)[source]

Implements support for spectral power distribution division.

Parameters:x (numeric or array_like or SpectralPowerDistribution) – Variable to divide.
Returns:Variable divided spectral power distribution.
Return type:SpectralPowerDistribution

See also

SpectralPowerDistribution.__add__(), SpectralPowerDistribution.__sub__(), SpectralPowerDistribution.__mul__()

Notes

  • Reimplements the object.__div__() method.

Warning

The division operation happens in place.

Examples

Dividing a single numeric variable:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd / 10  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 4.967,  6.959,  8.173,  8.819])

Dividing an array_like variable:

>>> spd / [1, 2, 3, 4]  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 4.967     ,  3.4795    ,  2.72433333,  2.20475   ])

Dividing a SpectralPowerDistribution class variable:

>>> spd_alternate = SpectralPowerDistribution('Spd', data)
>>> spd / spd_alternate  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values  
array([ 0.1       ,  0.05      ,  0.0333333...,  0.025     ])
__eq__(spd)[source]

Returns the spectral power distribution equality with given other spectral power distribution.

Parameters:spd (SpectralPowerDistribution) – Spectral power distribution to compare for equality.
Returns:Spectral power distribution equality.
Return type:bool

Notes

  • Reimplements the object.__eq__() method.

Examples

>>> data1 = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> data2 = {510: 48.6700, 520: 69.5900, 530: 81.7300, 540: 88.1900}
>>> spd1 = SpectralPowerDistribution('Spd', data1)
>>> spd2 = SpectralPowerDistribution('Spd', data2)
>>> spd3 = SpectralPowerDistribution('Spd', data2)
>>> spd1 == spd2
False
>>> spd2 == spd3
True
__getitem__(wavelength)[source]

Returns the value for given wavelength \(\lambda\).

Parameters:wavelength (numeric) – Wavelength \(\lambda\) to retrieve the value.
Returns:Wavelength \(\lambda\) value.
Return type:numeric

See also

SpectralPowerDistribution.get()

Notes

  • Reimplements the object.__getitem__() method.

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> spd[510]  
49.67...
__hash__()[source]

Returns the spectral power distribution hash value.

Returns:Object hash.
Return type:int

Notes

  • Reimplements the object.__hash__() method.

Warning

SpectralPowerDistribution class is mutable and should not be hashable. However, so that it can be used as a key in some data caches, we provide a __hash__ implementation, assuming that the underlying data will not change for those specific cases.

References

[1]http://stackoverflow.com/a/16162138/931625 (Last accessed 8 August 2014)
__iter__()[source]

Returns a generator for the spectral power distribution data.

Returns:Spectral power distribution data generator.
Return type:generator

Notes

  • Reimplements the object.__iter__() method.

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> for wavelength, value in spd: print((wavelength, value))    
(510, 49.6...)
(520, 69.5...)
(530, 81.7...)
(540, 88.1...)
__len__()[source]

Returns the spectral power distribution wavelengths \(\lambda_n\) count.

Returns:Spectral power distribution wavelengths \(\lambda_n\) count.
Return type:int

Notes

  • Reimplements the object.__len__() method.

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> len(spd)
4
__mul__(x)[source]

Implements support for spectral power distribution multiplication.

Parameters:x (numeric or array_like or SpectralPowerDistribution) – Variable to multiply.
Returns:Variable multiplied spectral power distribution.
Return type:SpectralPowerDistribution

See also

SpectralPowerDistribution.__add__(), SpectralPowerDistribution.__sub__(), SpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__mul__() method.

Warning

The multiplication operation happens in place.

Examples

Multiplying a single numeric variable:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd * 10  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 496.7,  695.9,  817.3,  881.9])

Multiplying an array_like variable:

>>> spd * [1, 2, 3, 4]  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([  496.7,  1391.8,  2451.9,  3527.6])

Multiplying a SpectralPowerDistribution class variable:

>>> spd_alternate = SpectralPowerDistribution('Spd', data)
>>> spd * spd_alternate  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([  24671.089,   96855.362,  200393.787,  311099.044])
__ne__(spd)[source]

Returns the spectral power distribution inequality with given other spectral power distribution.

Parameters:spd (SpectralPowerDistribution) – Spectral power distribution to compare for inequality.
Returns:Spectral power distribution inequality.
Return type:bool

Notes

  • Reimplements the object.__ne__() method.

Examples

>>> data1 = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> data2 = {510: 48.6700, 520: 69.5900, 530: 81.7300, 540: 88.1900}
>>> spd1 = SpectralPowerDistribution('Spd', data1)
>>> spd2 = SpectralPowerDistribution('Spd', data2)
>>> spd3 = SpectralPowerDistribution('Spd', data2)
>>> spd1 != spd2
True
>>> spd2 != spd3
False
__setitem__(wavelength, value)[source]

Sets the wavelength \(\lambda\) with given value.

Parameters:
  • wavelength (numeric) – Wavelength \(\lambda\) to set.
  • value (numeric) – Value for wavelength \(\lambda\).

Notes

  • Reimplements the object.__setitem__() method.

Examples

>>> spd = SpectralPowerDistribution('Spd', {})
>>> spd[510] = 49.6700
>>> spd.values
array([ 49.67])
__sub__(x)[source]

Implements support for spectral power distribution subtraction.

Parameters:x (numeric or array_like or SpectralPowerDistribution) – Variable to subtract.
Returns:Variable subtracted spectral power distribution.
Return type:SpectralPowerDistribution

See also

SpectralPowerDistribution.__add__(), SpectralPowerDistribution.__mul__(), SpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__sub__() method.

Warning

The subtraction operation happens in place.

Examples

Subtracting a single numeric variable:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd - 10  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 39.67,  59.59,  71.73,  78.19])

Subtracting an array_like variable:

>>> spd - [1, 2, 3, 4]  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 38.67,  57.59,  68.73,  74.19])

Subtracting a SpectralPowerDistribution class variable:

>>> spd_alternate = SpectralPowerDistribution('Spd', data)
>>> spd - spd_alternate  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([-11., -12., -13., -14.])
__truediv__(x)

Implements support for spectral power distribution division.

Parameters:x (numeric or array_like or SpectralPowerDistribution) – Variable to divide.
Returns:Variable divided spectral power distribution.
Return type:SpectralPowerDistribution

See also

SpectralPowerDistribution.__add__(), SpectralPowerDistribution.__sub__(), SpectralPowerDistribution.__mul__()

Notes

  • Reimplements the object.__div__() method.

Warning

The division operation happens in place.

Examples

Dividing a single numeric variable:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd / 10  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 4.967,  6.959,  8.173,  8.819])

Dividing an array_like variable:

>>> spd / [1, 2, 3, 4]  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([ 4.967     ,  3.4795    ,  2.72433333,  2.20475   ])

Dividing a SpectralPowerDistribution class variable:

>>> spd_alternate = SpectralPowerDistribution('Spd', data)
>>> spd / spd_alternate  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values  
array([ 0.1       ,  0.05      ,  0.0333333...,  0.025     ])
align(shape, method=u'Constant', left=None, right=None)[source]

Aligns the spectral power distribution to given spectral shape: Interpolates first then extrapolates to fit the given range.

Parameters:
  • shape (SpectralShape) – Spectral shape used for alignment.
  • method (unicode, optional) – (‘Linear’, ‘Constant’), Extrapolation method.
  • left (numeric, optional) – Value to return for low extrapolation range.
  • right (numeric, optional) – Value to return for high extrapolation range.
Returns:

Aligned spectral power distribution.
Return type:

SpectralPowerDistribution

See also

SpectralPowerDistribution.extrapolate(), SpectralPowerDistribution.interpolate()

Examples

>>> data = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 86.26,
...     560: 77.18}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.align(SpectralShape(505, 565, 1))  
<...SpectralPowerDistribution object at 0x...>
>>> # Doctests skip for Python 2.x compatibility.
>>> spd.wavelengths  
array([505, 506, 507, 508, 509, 510, 511, 512, 513, 514, 515, 516, 517,
       518, 519, 520, 521, 522, 523, 524, 525, 526, 527, 528, 529, 530,
       531, 532, 533, 534, 535, 536, 537, 538, 539, 540, 541, 542, 543,
       544, 545, 546, 547, 548, 549, 550, 551, 552, 553, 554, 555, 556,
       557, 558, 559, 560, 561, 562, 563, 564, 565])
>>> spd.values  
array([ 49.67     ...,  49.67     ...,  49.67     ...,  49.67     ...,
        49.67     ...,  49.67     ...,  51.8341162...,  53.9856467...,
        56.1229464...,  58.2366197...,  60.3121800...,  62.3327095...,
        64.2815187...,  66.1448055...,  67.9143153...,  69.59     ...,
        71.1759958...,  72.6627938...,  74.0465756...,  75.3329710...,
        76.5339542...,  77.6647421...,  78.7406907...,  79.7741932...,
        80.7715767...,  81.73     ...,  82.6407518...,  83.507872 ...,
        84.3326333...,  85.109696 ...,  85.8292968...,  86.47944  ...,
        87.0480863...,  87.525344 ...,  87.9056578...,  88.19     ...,
        88.3858347...,  88.4975634...,  88.5258906...,  88.4696570...,
        88.3266460...,  88.0943906...,  87.7709802...,  87.3558672...,
        86.8506741...,  86.26     ...,  85.5911699...,  84.8503430...,
        84.0434801...,  83.1771110...,  82.2583874...,  81.2951360...,
        80.2959122...,  79.2700525...,  78.2277286...,  77.18     ...,
        77.18     ...,  77.18     ...,  77.18     ...,  77.18     ...,  77.18      ])
clone()[source]

Clones the spectral power distribution.

Most of the SpectralPowerDistribution class operations are conducted in-place. The SpectralPowerDistribution.clone() method provides a convenient way to copy the spectral power distribution to a new object.

Returns:Cloned spectral power distribution.
Return type:SpectralPowerDistribution

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> print(spd)  
<...SpectralPowerDistribution object at 0x...>
>>> spd_clone = spd.clone()
>>> print(spd_clone)  
<...SpectralPowerDistribution object at 0x...>
data[source]

Property for self.__data private attribute.

Returns:self.__data.
Return type:dict
extrapolate(shape, method=u'Constant', left=None, right=None)[source]

Extrapolates the spectral power distribution following CIE 15:2004 recommendation.

Parameters:
  • shape (SpectralShape) – Spectral shape used for extrapolation.
  • method (unicode, optional) – (‘Linear’, ‘Constant’), Extrapolation method.
  • left (numeric, optional) – Value to return for low extrapolation range.
  • right (numeric, optional) – Value to return for high extrapolation range.
Returns:

Extrapolated spectral power distribution.
Return type:

SpectralPowerDistribution

See also

SpectralPowerDistribution.align()

References

[2]CIE 015:2004 Colorimetry, 3rd edition: 7.2.2.1 Extrapolation
[3]CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations: 10. EXTRAPOLATION

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.extrapolate(SpectralShape(400, 700)).shape
SpectralShape(400, 700, 10)
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> spd[400]  
49.67...
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> spd[700]  
88.1...
get(wavelength, default=None)[source]

Returns the value for given wavelength \(\lambda\).

Parameters:
  • wavelength (numeric) – Wavelength \(\lambda\) to retrieve the value.
  • default (None or numeric, optional) – Wavelength \(\lambda\) default value.
Returns:

Wavelength \(\lambda\) value.
Return type:

numeric

See also

SpectralPowerDistribution.__getitem__()

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> spd.get(510)  
49.67...
>>> spd.get(511)  
None
interpolate(shape=SpectralShape(None, None, None), method=None)[source]

Interpolates the spectral power distribution following CIE 167:2005 recommendations: the method developed by Sprague (1880) should be used for interpolating functions having a uniformly spaced independent variable and a Cubic Spline method for non-uniformly spaced independent variable.

Parameters:
  • shape (SpectralShape, optional) – Spectral shape used for interpolation.
  • method (unicode, optional) – (‘Sprague’, ‘Cubic Spline’, ‘Linear’), Enforce given interpolation method.
Returns:

Interpolated spectral power distribution.
Return type:

SpectralPowerDistribution
Raises:
  • RuntimeError – If the Sprague interpolation method is forced with a non-uniformly spaced independent variable.
  • ValueError – If the interpolation method is not defined.

See also

SpectralPowerDistribution.align()

Notes

Warning

  • If scipy is not unavailable the Cubic Spline method will fallback to legacy Linear interpolation.
  • Linear interpolator requires at least 2 wavelengths \(\lambda_n\) for interpolation.
  • Cubic Spline interpolator requires at least 3 wavelengths \(\lambda_n\) for interpolation.
  • Sprague interpolator requires at least 6 wavelengths \(\lambda_n\) for interpolation.

References

[4]CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations: 9. INTERPOLATION

Examples

Uniform data is using Sprague interpolation by default:

>>> data = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 86.26,
...     560: 77.18}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.interpolate(SpectralShape(steps=1))  
<...SpectralPowerDistribution object at 0x...>
>>> spd[515]  
60.3121800...

Non uniform data is using Cubic Spline interpolation by default:

>>> data = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 86.26,
...     560: 77.18}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd[511] = 31.41
>>> spd.interpolate(SpectralShape(steps=1))  
<...SpectralPowerDistribution object at 0x...>
>>> spd[515]  
21.4792222...

Enforcing Linear interpolation:

>>> data = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 86.26,
...     560: 77.18}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.interpolate(SpectralShape(steps=1), method='Linear')    
<...SpectralPowerDistribution object at 0x...>
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> spd[515]  
59.63...
is_uniform()[source]

Returns if the spectral power distribution has uniformly spaced data.

Returns:Is uniform.
Return type:bool

See also

SpectralPowerDistribution.shape()

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.is_uniform()
True

Breaking the steps by introducing a new wavelength \(\lambda\) value:

>>> spd[511] = 3.1415
>>> spd.is_uniform()
False
items[source]

Property for self.items attribute. This is a convenient attribute used to iterate over the spectral power distribution.

Returns:Spectral power distribution data generator.
Return type:generator
name[source]

Property for self.__name private attribute.

Returns:self.__name.
Return type:str or unicode
normalise(factor=1)[source]

Normalises the spectral power distribution with given normalization factor.

Parameters:factor (numeric, optional) – Normalization factor
Returns:Normalised spectral power distribution.
Return type:SpectralPowerDistribution

Examples

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.normalise()  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values  
array([ 0.5632157...,  0.7890917...,  0.9267490...,  1.        ])
shape[source]

Property for self.shape attribute.

Returns the shape of the spectral power distribution in the form of a SpectralShape class instance.

Returns:Spectral power distribution shape.
Return type:SpectralShape

See also

SpectralPowerDistribution.is_uniform

Notes

  • A non uniform spectral power distribution may will have multiple different steps, in that case SpectralPowerDistribution.shape returns the minimum steps size.

Warning

SpectralPowerDistribution.shape is read only.

Examples

Uniform spectral power distribution:

>>> data = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> SpectralPowerDistribution('Spd', data).shape
SpectralShape(510, 540, 10)

Non uniform spectral power distribution:

>>> data = {512.3: 49.67, 524.5: 69.59, 532.4: 81.73, 545.7: 88.19}
>>> # Doctests ellipsis for Python 2.x compatibility.
>>> SpectralPowerDistribution('Spd', data).shape  
SpectralShape(512.3, 545.7, 7...)
values[source]

Property for self.values attribute.

Returns:Spectral power distribution wavelengths \(\lambda_n\) values.
Return type:ndarray

Warning

SpectralPowerDistribution.values is read only.

wavelengths[source]

Property for self.wavelengths attribute.

Returns:Spectral power distribution wavelengths \(\lambda_n\).
Return type:ndarray

Warning

SpectralPowerDistribution.wavelengths is read only.

zeros(shape=SpectralShape(None, None, None))[source]

Zeros fills the spectral power distribution: Missing values will be replaced with zeros to fit the defined range.

Parameters:shape (SpectralShape, optional) – Spectral shape used for zeros fill.
Returns:Zeros filled spectral power distribution.
Return type:SpectralPowerDistribution

Examples

>>> data = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 86.26,
...     560: 77.18}
>>> spd = SpectralPowerDistribution('Spd', data)
>>> spd.zeros(SpectralShape(505, 565, 1))  
<...SpectralPowerDistribution object at 0x...>
>>> spd.values
array([  0.  ,   0.  ,   0.  ,   0.  ,   0.  ,  49.67,   0.  ,   0.  ,
         0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,  69.59,
         0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,
         0.  ,  81.73,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,
         0.  ,   0.  ,   0.  ,  88.19,   0.  ,   0.  ,   0.  ,   0.  ,
         0.  ,   0.  ,   0.  ,   0.  ,   0.  ,  86.26,   0.  ,   0.  ,
         0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,   0.  ,  77.18,
         0.  ,   0.  ,   0.  ,   0.  ,   0.  ])
class colour.colorimetry.spectrum.TriSpectralPowerDistribution(name, data, mapping, labels)[source]

Bases: object

Defines the base object for colour matching functions.

A compound of three SpectralPowerDistribution is used to store the underlying axis data.

Parameters:
  • name (str or unicode) – Tri-spectral power distribution name.
  • data (dict) – Tri-spectral power distribution data.
  • mapping (dict) – Tri-spectral power distribution attributes mapping.
  • labels (dict) – Tri-spectral power distribution axis labels mapping.
name[source]
mapping[source]
data[source]
labels[source]
x[source]
y[source]
z[source]
wavelengths[source]
values[source]
items[source]
shape[source]
__init__()[source]
__getitem__()[source]
__setitem__()[source]
__iter__()[source]
__contains__()[source]
__len__()[source]
__eq__()[source]
__ne__()[source]
__add__()[source]
__sub__()[source]
__mul__()[source]
__div__()[source]
__truediv__()
get()[source]
is_uniform()[source]
extrapolate()[source]
interpolate()[source]
align()[source]
zeros()[source]
normalise()[source]
clone()[source]

See also

colour.colorimetry.cmfs.LMS_ConeFundamentals, colour.colorimetry.cmfs.RGB_ColourMatchingFunctions, colour.colorimetry.cmfs.XYZ_ColourMatchingFunctions

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.wavelengths
array([510, 520, 530, 540])
>>> tri_spd.values
array([[ 49.67,  90.56,  12.43],
       [ 69.59,  87.34,  23.15],
       [ 81.73,  45.76,  67.98],
       [ 88.19,  23.45,  90.28]])
>>> tri_spd.shape
SpectralShape(510, 540, 10)
__add__(x)[source]

Implements support for tri-spectral power distribution addition.

Parameters:x (numeric or array_like or TriSpectralPowerDistribution) – Variable to add.
Returns:Variable added tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.__sub__(), TriSpectralPowerDistribution.__mul__(), TriSpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__add__() method.

Warning

The addition operation happens in place.

Examples

Adding a single numeric variable:

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd + 10  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  59.67,  100.56,   22.43],
       [  79.59,   97.34,   33.15],
       [  91.73,   55.76,   77.98],
       [  98.19,   33.45,  100.28]])

Adding an array_like variable:

>>> tri_spd + [(1, 2, 3)] * 4  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  60.67,  102.56,   25.43],
       [  80.59,   99.34,   36.15],
       [  92.73,   57.76,   80.98],
       [  99.19,   35.45,  103.28]])

Adding a TriSpectralPowerDistribution class variable:

>>> data1 = {'x_bar': z_bar, 'y_bar': x_bar, 'z_bar': y_bar}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd + tri_spd1  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  73.1 ,  152.23,  115.99],
       [ 103.74,  168.93,  123.49],
       [ 160.71,  139.49,  126.74],
       [ 189.47,  123.64,  126.73]])
__contains__(wavelength)[source]

Returns if the tri-spectral power distribution contains the given wavelength \(\lambda\).

Parameters:wavelength (numeric) – Wavelength \(\lambda\).
Returns:Is wavelength \(\lambda\) in the tri-spectral power distribution.
Return type:bool

Notes

  • Reimplements the object.__contains__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> 510 in tri_spd
True
__div__(x)[source]

Implements support for tri-spectral power distribution division.

Parameters:x (numeric or array_like or TriSpectralPowerDistribution) – Variable to divide.
Returns:Variable divided tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.__add__(), TriSpectralPowerDistribution.__sub__(), TriSpectralPowerDistribution.__mul__()

Notes

  • Reimplements the object.__mul__() method.

Warning

The division operation happens in place.

Examples

Dividing a single numeric variable:

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd / 10  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 4.967,  9.056,  1.243],
       [ 6.959,  8.734,  2.315],
       [ 8.173,  4.576,  6.798],
       [ 8.819,  2.345,  9.028]])

Dividing an array_like variable:

>>> tri_spd / [(1, 2, 3)] * 4  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values  
array([[ 19.868     ,  18.112     ,   1.6573333...],
       [ 27.836     ,  17.468     ,   3.0866666...],
       [ 32.692     ,   9.152     ,   9.064    ...],
       [ 35.276     ,   4.69      ,  12.0373333...]])

Dividing a TriSpectralPowerDistribution class variable:

>>> data1 = {'x_bar': z_bar, 'y_bar': x_bar, 'z_bar': y_bar}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd / tri_spd1  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values  
array([[ 1.5983909...,  0.3646466...,  0.0183009...],
       [ 1.2024190...,  0.2510130...,  0.0353408...],
       [ 0.4809061...,  0.1119784...,  0.1980769...],
       [ 0.3907399...,  0.0531806...,  0.5133191...]])
__eq__(tri_spd)[source]

Returns the tri-spectral power distribution equality with given other tri-spectral power distribution.

Parameters:spd (TriSpectralPowerDistribution) – Tri-spectral power distribution to compare for equality.
Returns:Tri-spectral power distribution equality.
Return type:bool

Notes

  • Reimplements the object.__eq__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data1 = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> data2 = {'x_bar': y_bar, 'y_bar': x_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd2 = TriSpectralPowerDistribution('Tri Spd', data2, mpg, lbl)
>>> tri_spd3 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd1 == tri_spd2
False
>>> tri_spd1 == tri_spd3
True
__getitem__(wavelength)[source]

Returns the values for given wavelength \(\lambda\).

Parameters:wavelength (numeric) – Wavelength \(\lambda\) to retrieve the values.
Returns:Wavelength \(\lambda\) values.
Return type:ndarray, (3,)

See also

TriSpectralPowerDistribution.get()

Notes

  • Reimplements the object.__getitem__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd[510]
array([ 49.67,  90.56,  12.43])
__hash__()[source]

Returns the spectral power distribution hash value.

Returns:Object hash.
Return type:int

Notes

  • Reimplements the object.__hash__() method.

Warning

See SpectralPowerDistribution.__hash__() method warning section.

References

[5]http://stackoverflow.com/a/16162138/931625 (Last accessed 8 August 2014)
__iter__()[source]

Returns a generator for the tri-spectral power distribution data.

Returns:Tri-spectral power distribution data generator.
Return type:generator

Notes

  • Reimplements the object.__iter__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> for wavelength, value in tri_spd: print((wavelength, value))
(510, array([ 49.67,  90.56,  12.43]))
(520, array([ 69.59,  87.34,  23.15]))
(530, array([ 81.73,  45.76,  67.98]))
(540, array([ 88.19,  23.45,  90.28]))
__len__()[source]

Returns the tri-spectral power distribution wavelengths \(\lambda_n\) count.

Returns:Tri-Spectral power distribution wavelengths \(\lambda_n\) count.
Return type:int

Notes

  • Reimplements the object.__len__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> len(tri_spd)
4
__mul__(x)[source]

Implements support for tri-spectral power distribution multiplication.

Parameters:x (numeric or array_like or TriSpectralPowerDistribution) – Variable to multiply.
Returns:Variable multiplied tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.__add__(), TriSpectralPowerDistribution.__sub__(), TriSpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__mul__() method.

Warning

The multiplication operation happens in place.

Examples

Multiplying a single numeric variable:

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd * 10  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 496.7,  905.6,  124.3],
       [ 695.9,  873.4,  231.5],
       [ 817.3,  457.6,  679.8],
       [ 881.9,  234.5,  902.8]])

Multiplying an array_like variable:

>>> tri_spd * [(1, 2, 3)] * 4  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  1986.8,   7244.8,   1491.6],
       [  2783.6,   6987.2,   2778. ],
       [  3269.2,   3660.8,   8157.6],
       [  3527.6,   1876. ,  10833.6]])

Multiplying a TriSpectralPowerDistribution class variable:

>>> data1 = {'x_bar': z_bar, 'y_bar': x_bar, 'z_bar': y_bar}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd * tri_spd1  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  24695.924,  359849.216,  135079.296],
       [  64440.34 ,  486239.248,  242630.52 ],
       [ 222240.216,  299197.184,  373291.776],
       [ 318471.728,  165444.44 ,  254047.92 ]])
__ne__(tri_spd)[source]

Returns the tri-spectral power distribution inequality with given other tri-spectral power distribution.

Parameters:spd (TriSpectralPowerDistribution) – Tri-spectral power distribution to compare for inequality.
Returns:Tri-spectral power distribution inequality.
Return type:bool

Notes

  • Reimplements the object.__eq__() method.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data1 = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> data2 = {'x_bar': y_bar, 'y_bar': x_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd2 = TriSpectralPowerDistribution('Tri Spd', data2, mpg, lbl)
>>> tri_spd3 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd1 != tri_spd2
True
>>> tri_spd1 != tri_spd3
False
__setitem__(wavelength, value)[source]

Sets the wavelength \(\lambda\) with given value.

Parameters:
  • wavelength (numeric) – Wavelength \(\lambda\) to set.
  • value (array_like) – Value for wavelength \(\lambda\).

Notes

  • Reimplements the object.__setitem__() method.

Examples

>>> x_bar = {}
>>> y_bar = {}
>>> z_bar = {}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd[510] = (49.6700, 49.6700, 49.6700)
>>> tri_spd.values
array([[ 49.67,  49.67,  49.67]])
__sub__(x)[source]

Implements support for tri-spectral power distribution subtraction.

Parameters:x (numeric or array_like or TriSpectralPowerDistribution) – Variable to subtract.
Returns:Variable subtracted tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.__add__(), TriSpectralPowerDistribution.__mul__(), TriSpectralPowerDistribution.__div__()

Notes

  • Reimplements the object.__sub__() method.

Warning

The subtraction operation happens in place.

Examples

Subtracting a single numeric variable:

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd - 10  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 39.67,  80.56,   2.43],
       [ 59.59,  77.34,  13.15],
       [ 71.73,  35.76,  57.98],
       [ 78.19,  13.45,  80.28]])

Subtracting an array_like variable:

>>> tri_spd - [(1, 2, 3)] * 4  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 38.67,  78.56,  -0.57],
       [ 58.59,  75.34,  10.15],
       [ 70.73,  33.76,  54.98],
       [ 77.19,  11.45,  77.28]])

Subtracting a TriSpectralPowerDistribution class variable:

>>> data1 = {'x_bar': z_bar, 'y_bar': x_bar, 'z_bar': y_bar}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd - tri_spd1  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 26.24,  28.89, -91.13],
       [ 35.44,   5.75, -77.19],
       [  2.75, -47.97,   9.22],
       [-13.09, -76.74,  53.83]])
__truediv__(x)

Implements support for tri-spectral power distribution division.

Parameters:x (numeric or array_like or TriSpectralPowerDistribution) – Variable to divide.
Returns:Variable divided tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.__add__(), TriSpectralPowerDistribution.__sub__(), TriSpectralPowerDistribution.__mul__()

Notes

  • Reimplements the object.__mul__() method.

Warning

The division operation happens in place.

Examples

Dividing a single numeric variable:

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd / 10  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[ 4.967,  9.056,  1.243],
       [ 6.959,  8.734,  2.315],
       [ 8.173,  4.576,  6.798],
       [ 8.819,  2.345,  9.028]])

Dividing an array_like variable:

>>> tri_spd / [(1, 2, 3)] * 4  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values  
array([[ 19.868     ,  18.112     ,   1.6573333...],
       [ 27.836     ,  17.468     ,   3.0866666...],
       [ 32.692     ,   9.152     ,   9.064    ...],
       [ 35.276     ,   4.69      ,  12.0373333...]])

Dividing a TriSpectralPowerDistribution class variable:

>>> data1 = {'x_bar': z_bar, 'y_bar': x_bar, 'z_bar': y_bar}
>>> tri_spd1 = TriSpectralPowerDistribution('Tri Spd', data1, mpg, lbl)
>>> tri_spd / tri_spd1  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values  
array([[ 1.5983909...,  0.3646466...,  0.0183009...],
       [ 1.2024190...,  0.2510130...,  0.0353408...],
       [ 0.4809061...,  0.1119784...,  0.1980769...],
       [ 0.3907399...,  0.0531806...,  0.5133191...]])
align(shape, method=u'Constant', left=None, right=None)[source]

Aligns the tri-spectral power distribution to given shape: Interpolates first then extrapolates to fit the given range.

Parameters:
  • shape (SpectralShape) – Spectral shape used for alignment.
  • method (unicode, optional) – (‘Linear’, ‘Constant’), Extrapolation method.
  • left (numeric, optional) – Value to return for low extrapolation range.
  • right (numeric, optional) – Value to return for high extrapolation range.
Returns:

Aligned tri-spectral power distribution.
Return type:

TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.extrapolate(), TriSpectralPowerDistribution.interpolate()

Examples

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.align(SpectralShape(505, 565, 1))  
<...TriSpectralPowerDistribution object at 0x...>
>>> # Doctests skip for Python 2.x compatibility.
>>> tri_spd.wavelengths  
array([505, 506, 507, 508, 509, 510, 511, 512, 513, 514, 515, 516, 517,
       518, 519, 520, 521, 522, 523, 524, 525, 526, 527, 528, 529, 530,
       531, 532, 533, 534, 535, 536, 537, 538, 539, 540, 541, 542, 543,
       544, 545, 546, 547, 548, 549, 550, 551, 552, 553, 554, 555, 556,
       557, 558, 559, 560, 561, 562, 563, 564, 565])
>>> tri_spd.values  
array([[ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 49.67     ...,  90.56     ...,  12.43     ...],
       [ 51.8325938...,  91.2994928...,  12.5377184...],
       [ 53.9841952...,  91.9502387...,  12.7233193...],
       [ 56.1205452...,  92.5395463...,  12.9651679...],
       [ 58.2315395...,  93.0150037...,  13.3123777...],
       [ 60.3033208...,  93.2716331...,  13.8605136...],
       [ 62.3203719...,  93.1790455...,  14.7272944...],
       [ 64.2676077...,  92.6085951...,  16.0282961...],
       [ 66.1324679...,  91.4605335...,  17.8526544...],
       [ 67.9070097...,  89.6911649...,  20.2387677...],
       [ 69.59     ...,  87.34     ...,  23.15     ...],
       [ 71.1837378...,  84.4868033...,  26.5150469...],
       [ 72.6800056...,  81.0666018...,  30.3964852...],
       [ 74.0753483...,  77.0766254...,  34.7958422...],
       [ 75.3740343...,  72.6153870...,  39.6178858...],
       [ 76.5856008...,  67.8490714...,  44.7026805...],
       [ 77.7223995...,  62.9779261...,  49.8576432...],
       [ 78.7971418...,  58.2026503...,  54.8895997...],
       [ 79.8204447...,  53.6907852...,  59.6368406...],
       [ 80.798376 ...,  49.5431036...,  64.0011777...],
       [ 81.73     ...,  45.76     ...,  67.98     ...],
       [ 82.6093606...,  42.2678534...,  71.6460893...],
       [ 83.439232 ...,  39.10608  ...,  74.976976 ...],
       [ 84.2220071...,  36.3063728...,  77.9450589...],
       [ 84.956896 ...,  33.85464  ...,  80.552    ...],
       [ 85.6410156...,  31.7051171...,  82.8203515...],
       [ 86.27048  ...,  29.79448  ...,  84.785184 ...],
       [ 86.8414901...,  28.0559565...,  86.4857131...],
       [ 87.351424 ...,  26.43344  ...,  87.956928 ...],
       [ 87.7999266...,  24.8956009...,  89.2212178...],
       [ 88.19     ...,  23.45     ...,  90.28     ...],
       [ 88.5265036...,  22.1424091...,  91.1039133...],
       [ 88.8090803...,  20.9945234...,  91.6538035...],
       [ 89.0393279...,  20.0021787...,  91.9333499...],
       [ 89.2222817...,  19.1473370...,  91.9858818...],
       [ 89.3652954...,  18.4028179...,  91.8811002...],
       [ 89.4769231...,  17.7370306...,  91.7018000...],
       [ 89.5657996...,  17.1187058...,  91.5305910...],
       [ 89.6395227...,  16.5216272...,  91.4366204...],
       [ 89.7035339...,  15.9293635...,  91.4622944...],
       [ 89.76     ...,  15.34     ...,  91.61     ...],
       [ 89.8094041...,  14.7659177...,  91.8528616...],
       [ 89.8578890...,  14.2129190...,  92.2091737...],
       [ 89.9096307...,  13.6795969...,  92.6929664...],
       [ 89.9652970...,  13.1613510...,  93.2988377...],
       [ 90.0232498...,  12.6519811...,  94.0078786...],
       [ 90.0807467...,  12.1452800...,  94.7935995...],
       [ 90.1351435...,  11.6366269...,  95.6278555...],
       [ 90.1850956...,  11.1245805...,  96.4867724...],
       [ 90.2317606...,  10.6124724...,  97.3566724...],
       [ 90.28     ...,  10.11     ...,  98.24     ...],
       [ 90.28     ...,  10.11     ...,  98.24     ...],
       [ 90.28     ...,  10.11     ...,  98.24     ...],
       [ 90.28     ...,  10.11     ...,  98.24     ...],
       [ 90.28     ...,  10.11     ...,  98.24     ...],
       [ 90.28     ...,  10.11     ...,  98.24     ...]])
clone()[source]

Clones the tri-spectral power distribution.

Most of the TriSpectralPowerDistribution class operations are conducted in-place. The TriSpectralPowerDistribution.clone() method provides a convenient way to copy the tri-spectral power distribution to a new object.

Returns:Cloned tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

Examples

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> print(tri_spd)  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd_clone = tri_spd.clone()
>>> print(tri_spd_clone)  
<...TriSpectralPowerDistribution object at 0x...>
data[source]

Property for self.__data private attribute.

Returns:self.__data.
Return type:dict
extrapolate(shape, method=u'Constant', left=None, right=None)[source]

Extrapolates the tri-spectral power distribution following CIE 15:2004 recommendation.

Parameters:
  • shape (SpectralShape) – Spectral shape used for extrapolation.
  • method (unicode, optional) – (‘Linear’, ‘Constant’), Extrapolation method.
  • left (numeric, optional) – Value to return for low extrapolation range.
  • right (numeric, optional) – Value to return for high extrapolation range.
Returns:

Extrapolated tri-spectral power distribution.
Return type:

TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.align()

References

[6]CIE 015:2004 Colorimetry, 3rd edition: 7.2.2.1 Extrapolation
[7]CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations: 10. EXTRAPOLATION

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.extrapolate(SpectralShape(400, 700)).shape
SpectralShape(400, 700, 10)
>>> tri_spd[400]
array([ 49.67,  90.56,  12.43])
>>> tri_spd[700]
array([ 88.19,  23.45,  90.28])
get(wavelength, default=None)[source]

Returns the values for given wavelength \(\lambda\).

Parameters:
  • wavelength (numeric) – Wavelength \(\lambda\) to retrieve the values.
  • default (None or numeric, optional) – Wavelength \(\lambda\) default values.
Returns:

Wavelength \(\lambda\) values.
Return type:

numeric

See also

TriSpectralPowerDistribution.__getitem__()

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd[510]
array([ 49.67,  90.56,  12.43])
>>> tri_spd.get(511)  
None
interpolate(shape=SpectralShape(None, None, None), method=None)[source]

Interpolates the tri-spectral power distribution following CIE 167:2005 recommendations: the method developed by Sprague (1880) should be used for interpolating functions having a uniformly spaced independent variable and a Cubic Spline method for non-uniformly spaced independent variable.

Parameters:
  • shape (SpectralShape, optional) – Spectral shape used for interpolation.
  • method (unicode, optional) – (‘Sprague’, ‘Cubic Spline’, ‘Linear’), Enforce given interpolation method.
Returns:

Interpolated tri-spectral power distribution.
Return type:

TriSpectralPowerDistribution

See also

TriSpectralPowerDistribution.align()

Notes

Warning

See SpectralPowerDistribution.interpolate() method warning section.

References

[4]CIE 167:2005 Recommended Practice for Tabulating Spectral Data for Use in Colour Computations: 9. INTERPOLATION

Examples

Uniform data is using Sprague interpolation by default:

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.interpolate(SpectralShape(steps=1))  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd[515]
array([ 60.30332087,  93.27163315,  13.86051361])

Non uniform data is using Cubic Spline interpolation by default:

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd[511] = (31.41, 95.27, 15.06)
>>> tri_spd.interpolate(SpectralShape(steps=1))  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd[515]
array([  21.47104053,  100.64300155,   18.8165196 ])

Enforcing Linear interpolation:

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.interpolate(SpectralShape(steps=1), method='Linear')    
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd[515]
array([ 59.63,  88.95,  17.79])
is_uniform()[source]

Returns if the tri-spectral power distribution has uniformly spaced data.

Returns:Is uniform.
Return type:bool

See also

TriSpectralPowerDistribution.shape()

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.is_uniform()
True

Breaking the steps by introducing new wavelength \(\lambda\) values:

>>> tri_spd[511] = (49.6700, 49.6700, 49.6700)
>>> tri_spd.is_uniform()
False
items[source]

Property for self.items attribute. This is a convenient attribute used to iterate over the tri-spectral power distribution.

Returns:Tri-spectral power distribution data generator.
Return type:generator
labels[source]

Property for self.__labels private attribute.

Returns:self.__labels.
Return type:dict
mapping[source]

Property for self.__mapping private attribute.

Returns:self.__mapping.
Return type:dict
name[source]

Property for self.__name private attribute.

Returns:self.__name.
Return type:str or unicode
normalise(factor=1)[source]

Normalises the tri-spectral power distribution with given normalization factor.

Parameters:factor (numeric, optional) – Normalization factor
Returns:Normalised tri- spectral power distribution.
Return type:TriSpectralPowerDistribution

Notes

  • The implementation uses the maximum value for all axis.

Examples

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.normalise()  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values  
array([[ 0.5055985...,  0.9218241...,  0.1265268...],
       [ 0.7083672...,  0.8890472...,  0.2356473...],
       [ 0.8319421...,  0.4657980...,  0.6919788...],
       [ 0.8976995...,  0.2387011...,  0.9189739...],
       [ 0.9136807...,  0.1561482...,  0.9325122...],
       [ 0.9189739...,  0.1029112...,  1.       ...]])
shape[source]

Property for self.shape attribute.

Returns the shape of the tri-spectral power distribution in the form of a SpectralShape class instance.

Returns:Tri-spectral power distribution shape.
Return type:SpectralShape

See also

SpectralPowerDistribution.is_uniform, TriSpectralPowerDistribution.is_uniform

Warning

TriSpectralPowerDistribution.shape is read only.

Examples

>>> x_bar = {510: 49.67, 520: 69.59, 530: 81.73, 540: 88.19}
>>> y_bar = {510: 90.56, 520: 87.34, 530: 45.76, 540: 23.45}
>>> z_bar = {510: 12.43, 520: 23.15, 530: 67.98, 540: 90.28}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.shape
SpectralShape(510, 540, 10)
values[source]

Property for self.values attribute.

Returns:Tri-spectral power distribution wavelengths \(\lambda_n\) values.
Return type:ndarray

Warning

TriSpectralPowerDistribution.values is read only.

wavelengths[source]

Property for self.wavelengths attribute.

Returns:Tri-spectral power distribution wavelengths \(\lambda_n\).
Return type:ndarray

Warning

TriSpectralPowerDistribution.wavelengths is read only.

x[source]

Property for self.x attribute.

Returns:Spectral power distribution for x axis.
Return type:SpectralPowerDistribution

Warning

TriSpectralPowerDistribution.x is read only.

y[source]

Property for self.y attribute.

Returns:Spectral power distribution for y axis.
Return type:SpectralPowerDistribution

Warning

TriSpectralPowerDistribution.y is read only.

z[source]

Property for self.z attribute.

Returns:Spectral power distribution for z axis.
Return type:SpectralPowerDistribution

Warning

TriSpectralPowerDistribution.z is read only.

zeros(shape=SpectralShape(None, None, None))[source]

Zeros fills the tri-spectral power distribution: Missing values will be replaced with zeros to fit the defined range.

Parameters:shape (SpectralShape, optional) – Spectral shape used for zeros fill.
Returns:Zeros filled tri-spectral power distribution.
Return type:TriSpectralPowerDistribution

Examples

>>> x_bar = {
...     510: 49.67,
...     520: 69.59,
...     530: 81.73,
...     540: 88.19,
...     550: 89.76,
...     560: 90.28}
>>> y_bar = {
...     510: 90.56,
...     520: 87.34,
...     530: 45.76,
...     540: 23.45,
...     550: 15.34,
...     560: 10.11}
>>> z_bar = {
...     510: 12.43,
...     520: 23.15,
...     530: 67.98,
...     540: 90.28,
...     550: 91.61,
...     560: 98.24}
>>> data = {'x_bar': x_bar, 'y_bar': y_bar, 'z_bar': z_bar}
>>> mpg = lbl = {'x': 'x_bar', 'y': 'y_bar', 'z': 'z_bar'}
>>> tri_spd = TriSpectralPowerDistribution('Tri Spd', data, mpg, lbl)
>>> tri_spd.zeros(SpectralShape(505, 565, 1))  
<...TriSpectralPowerDistribution object at 0x...>
>>> tri_spd.values
array([[  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 49.67,  90.56,  12.43],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 69.59,  87.34,  23.15],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 81.73,  45.76,  67.98],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 88.19,  23.45,  90.28],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 89.76,  15.34,  91.61],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [ 90.28,  10.11,  98.24],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ],
       [  0.  ,   0.  ,   0.  ]])
colour.colorimetry.spectrum.DEFAULT_SPECTRAL_SHAPE = SpectralShape(360, 830, 1)

Default spectral shape using the shape of CIE 1931 2 Degree Standard Observer.

DEFAULT_SPECTRAL_SHAPE : SpectralShape

colour.colorimetry.spectrum.constant_spd(k, shape=SpectralShape(360, 830, 1))[source]

Returns a spectral power distribution of given spectral shape filled with constant \(k\) values.

Parameters:
  • k (numeric) – Constant \(k\) to fill the spectral power distribution with.
  • shape (SpectralShape, optional) – Spectral shape used to create the spectral power distribution.
Returns:

Constant \(k\) to filled spectral power distribution.
Return type:

SpectralPowerDistribution

Notes

Examples

>>> spd = constant_spd(100)
>>> spd.shape
SpectralShape(360, 830, 1)
>>> spd[400]
100.0
colour.colorimetry.spectrum.zeros_spd(shape=SpectralShape(360, 830, 1))[source]

Returns a spectral power distribution of given spectral shape filled with zeros.

Parameters:shape (SpectralShape, optional) – Spectral shape used to create the spectral power distribution.
Returns:Zeros filled spectral power distribution.
Return type:SpectralPowerDistribution

See also

constant_spd()

Notes

Examples

>>> spd = zeros_spd()
>>> spd.shape
SpectralShape(360, 830, 1)
>>> spd[400]
0.0
colour.colorimetry.spectrum.ones_spd(shape=SpectralShape(360, 830, 1))[source]

Returns a spectral power distribution of given spectral shape filled with ones.

Parameters:shape (SpectralShape, optional) – Spectral shape used to create the spectral power distribution.
Returns:Ones filled spectral power distribution.
Return type:SpectralPowerDistribution

See also

constant_spd()

Notes

Examples

>>> spd = ones_spd()
>>> spd.shape
SpectralShape(360, 830, 1)
>>> spd[400]
1.0