colour.SpectralDistribution¶
- class colour.SpectralDistribution(data: Optional[Union[ArrayLike, dict, Series, Signal, SpectralDistribution]] = None, domain: Optional[Union[ArrayLike, SpectralShape]] = None, **kwargs: Any)[source]¶
Bases:
colour.continuous.signal.Signal
Define the spectral distribution: the base object for spectral computations.
The spectral distribution will be initialised according to CIE 15:2004 recommendation: the method developed by Sprague (1880) will be used for interpolating functions having a uniformly spaced independent variable and the Cubic Spline method for non-uniformly spaced independent variable. Extrapolation is performed according to CIE 167:2005 recommendation.
Important
Specific documentation about getting, setting, indexing and slicing the spectral power distribution values is available in the Spectral Representation and Continuous Signal section.
- Parameters
data (Optional[Union[ArrayLike, dict, Series, Signal, SpectralDistribution]]) – Data to be stored in the spectral distribution.
domain (Optional[Union[ArrayLike, SpectralShape]]) – Values to initialise the
colour.SpectralDistribution.wavelength
property with. If bothdata
anddomain
arguments are defined, the latter will be used to initialise thecolour.SpectralDistribution.wavelength
property.extrapolator – Extrapolator class type to use as extrapolating function.
extrapolator_kwargs – Arguments to use when instantiating the extrapolating function.
interpolator – Interpolator class type to use as interpolating function.
interpolator_kwargs – Arguments to use when instantiating the interpolating function.
name – Spectral distribution name.
strict_name – Spectral distribution name for figures, default to
colour.SpectralDistribution.name
property value.kwargs (Any) –
Attributes
Methods
References
[CIET13805a], [CIET13805c], [CIET14804h]
Examples
Instantiating a spectral distribution with a uniformly spaced independent variable:
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> with numpy_print_options(suppress=True): ... SpectralDistribution(data) SpectralDistribution([[ 500. , 0.0651], [ 520. , 0.0705], [ 540. , 0.0772], [ 560. , 0.087 ], [ 580. , 0.1128], [ 600. , 0.136 ]], interpolator=SpragueInterpolator, interpolator_kwargs={}, extrapolator=Extrapolator, extrapolator_kwargs={...})
Instantiating a spectral distribution with a non-uniformly spaced independent variable:
>>> data[510] = 0.31416 >>> with numpy_print_options(suppress=True): ... SpectralDistribution(data) SpectralDistribution([[ 500. , 0.0651 ], [ 510. , 0.31416], [ 520. , 0.0705 ], [ 540. , 0.0772 ], [ 560. , 0.087 ], [ 580. , 0.1128 ], [ 600. , 0.136 ]], interpolator=CubicSplineInterpolator, interpolator_kwargs={}, extrapolator=Extrapolator, extrapolator_kwargs={...})
Instantiation with a Pandas
pandas.Series
:>>> from colour.utilities import is_pandas_installed >>> if is_pandas_installed(): ... from pandas import Series ... print(SpectralDistribution(Series(data))) [[ 5.0000000...e+02 6.5100000...e-02] [ 5.2000000...e+02 7.0500000...e-02] [ 5.4000000...e+02 7.7200000...e-02] [ 5.6000000...e+02 8.7000000...e-02] [ 5.8000000...e+02 1.1280000...e-01] [ 6.0000000...e+02 1.3600000...e-01] [ 5.1000000...e+02 3.1416000...e-01]]
- __init__(data: Optional[Union[ArrayLike, dict, Series, Signal, SpectralDistribution]] = None, domain: Optional[Union[ArrayLike, SpectralShape]] = None, **kwargs: Any)[source]¶
- Parameters
data (Optional[Union[ArrayLike, dict, Series, Signal, SpectralDistribution]]) –
domain (Optional[Union[ArrayLike, SpectralShape]]) –
kwargs (Any) –
- property strict_name: str¶
Getter and setter property for the spectral distribution strict name.
- Parameters
value – Value to set the spectral distribution strict name with.
- Returns
Spectral distribution strict name.
- Return type
- property wavelengths: numpy.ndarray¶
Getter and setter property for the spectral distribution wavelengths \(\lambda_n\).
- Parameters
value – Value to set the spectral distribution wavelengths \(\lambda_n\) with.
- Returns
Spectral distribution wavelengths \(\lambda_n\).
- Return type
- property values: numpy.ndarray¶
Getter and setter property for the spectral distribution values.
- Parameters
value – Value to set the spectral distribution wavelengths values with.
- Returns
Spectral distribution values.
- Return type
- property shape: colour.colorimetry.spectrum.SpectralShape¶
Getter property for the spectral distribution shape.
- Returns
Spectral distribution shape.
- Return type
Notes
A spectral distribution with a non-uniformly spaced independent variable have multiple intervals, in that case
colour.SpectralDistribution.shape
property returns the minimum interval size.
Examples
Shape of a spectral distribution with a uniformly spaced independent variable:
>>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> SpectralDistribution(data).shape SpectralShape(500.0, 600.0, 20.0)
Shape of a spectral distribution with a non-uniformly spaced independent variable:
>>> data[510] = 0.31416 >>> SpectralDistribution(data).shape SpectralShape(500.0, 600.0, 10.0)
- interpolate(shape: colour.colorimetry.spectrum.SpectralShape, interpolator: Optional[Type[colour.hints.TypeInterpolator]] = None, interpolator_kwargs: Optional[Dict] = None) colour.colorimetry.spectrum.SpectralDistribution [source]¶
Interpolate the spectral distribution in-place according to CIE 167:2005 recommendation (if the interpolator has not been changed at instantiation time) or given interpolation arguments.
The logic for choosing the interpolator class when
interpolator
is not given is as follows:if self.interpolator not in (SpragueInterpolator, CubicSplineInterpolator): interpolator = self.interpolator elif self.is_uniform(): interpolator = SpragueInterpolator else: interpolator = CubicSplineInterpolator
The logic for choosing the interpolator keyword arguments when
interpolator_kwargs
is not given is as follows:if self.interpolator not in (SpragueInterpolator, CubicSplineInterpolator): interpolator_kwargs = self.interpolator_kwargs else: interpolator_kwargs = {}
- Parameters
shape (colour.colorimetry.spectrum.SpectralShape) – Spectral shape used for interpolation.
interpolator (Optional[Type[colour.hints.TypeInterpolator]]) – Interpolator class type to use as interpolating function.
interpolator_kwargs (Optional[Dict]) – Arguments to use when instantiating the interpolating function.
- Returns
Interpolated spectral distribution.
- Return type
Notes
Interpolation will be performed over boundaries range, if you need to extend the range of the spectral distribution use the
colour.SpectralDistribution.extrapolate()
orcolour.SpectralDistribution.align()
methods.
Warning
Cubic Spline interpolator requires at least 3 wavelengths \(\lambda_n\) for interpolation.
Sprague (1880) interpolator requires at least 6 wavelengths \(\lambda_n\) for interpolation.
References
Examples
Spectral distribution with a uniformly spaced independent variable uses Sprague (1880) interpolation:
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> sd = SpectralDistribution(data) >>> with numpy_print_options(suppress=True): ... print(sd.interpolate(SpectralShape(500, 600, 1))) ... [[ 500. 0.0651 ...] [ 501. 0.0653522...] [ 502. 0.0656105...] [ 503. 0.0658715...] [ 504. 0.0661328...] [ 505. 0.0663929...] [ 506. 0.0666509...] [ 507. 0.0669069...] [ 508. 0.0671613...] [ 509. 0.0674150...] [ 510. 0.0676692...] [ 511. 0.0679253...] [ 512. 0.0681848...] [ 513. 0.0684491...] [ 514. 0.0687197...] [ 515. 0.0689975...] [ 516. 0.0692832...] [ 517. 0.0695771...] [ 518. 0.0698787...] [ 519. 0.0701870...] [ 520. 0.0705 ...] [ 521. 0.0708155...] [ 522. 0.0711336...] [ 523. 0.0714547...] [ 524. 0.0717789...] [ 525. 0.0721063...] [ 526. 0.0724367...] [ 527. 0.0727698...] [ 528. 0.0731051...] [ 529. 0.0734423...] [ 530. 0.0737808...] [ 531. 0.0741203...] [ 532. 0.0744603...] [ 533. 0.0748006...] [ 534. 0.0751409...] [ 535. 0.0754813...] [ 536. 0.0758220...] [ 537. 0.0761633...] [ 538. 0.0765060...] [ 539. 0.0768511...] [ 540. 0.0772 ...] [ 541. 0.0775527...] [ 542. 0.0779042...] [ 543. 0.0782507...] [ 544. 0.0785908...] [ 545. 0.0789255...] [ 546. 0.0792576...] [ 547. 0.0795917...] [ 548. 0.0799334...] [ 549. 0.0802895...] [ 550. 0.0806671...] [ 551. 0.0810740...] [ 552. 0.0815176...] [ 553. 0.0820049...] [ 554. 0.0825423...] [ 555. 0.0831351...] [ 556. 0.0837873...] [ 557. 0.0845010...] [ 558. 0.0852763...] [ 559. 0.0861110...] [ 560. 0.087 ...] [ 561. 0.0879383...] [ 562. 0.0889300...] [ 563. 0.0899793...] [ 564. 0.0910876...] [ 565. 0.0922541...] [ 566. 0.0934760...] [ 567. 0.0947487...] [ 568. 0.0960663...] [ 569. 0.0974220...] [ 570. 0.0988081...] [ 571. 0.1002166...] [ 572. 0.1016394...] [ 573. 0.1030687...] [ 574. 0.1044972...] [ 575. 0.1059186...] [ 576. 0.1073277...] [ 577. 0.1087210...] [ 578. 0.1100968...] [ 579. 0.1114554...] [ 580. 0.1128 ...] [ 581. 0.1141333...] [ 582. 0.1154495...] [ 583. 0.1167424...] [ 584. 0.1180082...] [ 585. 0.1192452...] [ 586. 0.1204536...] [ 587. 0.1216348...] [ 588. 0.1227915...] [ 589. 0.1239274...] [ 590. 0.1250465...] [ 591. 0.1261531...] [ 592. 0.1272517...] [ 593. 0.1283460...] [ 594. 0.1294393...] [ 595. 0.1305340...] [ 596. 0.1316310...] [ 597. 0.1327297...] [ 598. 0.1338277...] [ 599. 0.1349201...] [ 600. 0.136 ...]]
Spectral distribution with a non-uniformly spaced independent variable uses Cubic Spline interpolation:
>>> sd = SpectralDistribution(data) >>> sd[510] = np.pi / 10 >>> with numpy_print_options(suppress=True): ... print(sd.interpolate(SpectralShape(500, 600, 1))) ... [[ 500. 0.0651 ...] [ 501. 0.1365202...] [ 502. 0.1953263...] [ 503. 0.2423724...] [ 504. 0.2785126...] [ 505. 0.3046010...] [ 506. 0.3214916...] [ 507. 0.3300387...] [ 508. 0.3310962...] [ 509. 0.3255184...] [ 510. 0.3141592...] [ 511. 0.2978729...] [ 512. 0.2775135...] [ 513. 0.2539351...] [ 514. 0.2279918...] [ 515. 0.2005378...] [ 516. 0.1724271...] [ 517. 0.1445139...] [ 518. 0.1176522...] [ 519. 0.0926962...] [ 520. 0.0705 ...] [ 521. 0.0517370...] [ 522. 0.0363589...] [ 523. 0.0241365...] [ 524. 0.0148407...] [ 525. 0.0082424...] [ 526. 0.0041126...] [ 527. 0.0022222...] [ 528. 0.0023421...] [ 529. 0.0042433...] [ 530. 0.0076966...] [ 531. 0.0124729...] [ 532. 0.0183432...] [ 533. 0.0250785...] [ 534. 0.0324496...] [ 535. 0.0402274...] [ 536. 0.0481829...] [ 537. 0.0560870...] [ 538. 0.0637106...] [ 539. 0.0708246...] [ 540. 0.0772 ...] [ 541. 0.0826564...] [ 542. 0.0872086...] [ 543. 0.0909203...] [ 544. 0.0938549...] [ 545. 0.0960760...] [ 546. 0.0976472...] [ 547. 0.0986321...] [ 548. 0.0990942...] [ 549. 0.0990971...] [ 550. 0.0987043...] [ 551. 0.0979794...] [ 552. 0.0969861...] [ 553. 0.0957877...] [ 554. 0.0944480...] [ 555. 0.0930304...] [ 556. 0.0915986...] [ 557. 0.0902161...] [ 558. 0.0889464...] [ 559. 0.0878532...] [ 560. 0.087 ...] [ 561. 0.0864371...] [ 562. 0.0861623...] [ 563. 0.0861600...] [ 564. 0.0864148...] [ 565. 0.0869112...] [ 566. 0.0876336...] [ 567. 0.0885665...] [ 568. 0.0896945...] [ 569. 0.0910020...] [ 570. 0.0924735...] [ 571. 0.0940936...] [ 572. 0.0958467...] [ 573. 0.0977173...] [ 574. 0.0996899...] [ 575. 0.1017491...] [ 576. 0.1038792...] [ 577. 0.1060649...] [ 578. 0.1082906...] [ 579. 0.1105408...] [ 580. 0.1128 ...] [ 581. 0.1150526...] [ 582. 0.1172833...] [ 583. 0.1194765...] [ 584. 0.1216167...] [ 585. 0.1236884...] [ 586. 0.1256760...] [ 587. 0.1275641...] [ 588. 0.1293373...] [ 589. 0.1309798...] [ 590. 0.1324764...] [ 591. 0.1338114...] [ 592. 0.1349694...] [ 593. 0.1359349...] [ 594. 0.1366923...] [ 595. 0.1372262...] [ 596. 0.1375211...] [ 597. 0.1375614...] [ 598. 0.1373316...] [ 599. 0.1368163...] [ 600. 0.136 ...]]
- extrapolate(shape: colour.colorimetry.spectrum.SpectralShape, extrapolator: Optional[Type[colour.hints.TypeExtrapolator]] = None, extrapolator_kwargs: Optional[Dict] = None) colour.colorimetry.spectrum.SpectralDistribution [source]¶
Extrapolate the spectral distribution in-place according to CIE 15:2004 and CIE 167:2005 recommendations or given extrapolation arguments.
- Parameters
shape (colour.colorimetry.spectrum.SpectralShape) – Spectral shape used for extrapolation.
extrapolator (Optional[Type[colour.hints.TypeExtrapolator]]) – Extrapolator class type to use as extrapolating function.
extrapolator_kwargs (Optional[Dict]) – Arguments to use when instantiating the extrapolating function.
- Returns
Extrapolated spectral distribution.
- Return type
References
[CIET13805c], [CIET14804h]
Examples
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> sd = SpectralDistribution(data) >>> sd.extrapolate(SpectralShape(400, 700, 20)).shape SpectralShape(400.0, 700.0, 20.0) >>> with numpy_print_options(suppress=True): ... print(sd) [[ 400. 0.0651] [ 420. 0.0651] [ 440. 0.0651] [ 460. 0.0651] [ 480. 0.0651] [ 500. 0.0651] [ 520. 0.0705] [ 540. 0.0772] [ 560. 0.087 ] [ 580. 0.1128] [ 600. 0.136 ] [ 620. 0.136 ] [ 640. 0.136 ] [ 660. 0.136 ] [ 680. 0.136 ] [ 700. 0.136 ]]
- align(shape: colour.colorimetry.spectrum.SpectralShape, interpolator: Optional[Type[colour.hints.TypeInterpolator]] = None, interpolator_kwargs: Optional[Dict] = None, extrapolator: Optional[Type[colour.hints.TypeExtrapolator]] = None, extrapolator_kwargs: Optional[Dict] = None) colour.colorimetry.spectrum.SpectralDistribution [source]¶
Align the spectral distribution in-place to given spectral shape: Interpolates first then extrapolates to fit the given range.
Interpolation is performed according to CIE 167:2005 recommendation (if the interpolator has not been changed at instantiation time) or given interpolation arguments.
The logic for choosing the interpolator class when
interpolator
is not given is as follows:if self.interpolator not in (SpragueInterpolator, CubicSplineInterpolator): interpolator = self.interpolator elif self.is_uniform(): interpolator = SpragueInterpolator else: interpolator = CubicSplineInterpolator
The logic for choosing the interpolator keyword arguments when
interpolator_kwargs
is not given is as follows:if self.interpolator not in (SpragueInterpolator, CubicSplineInterpolator): interpolator_kwargs = self.interpolator_kwargs else: interpolator_kwargs = {}
- Parameters
shape (colour.colorimetry.spectrum.SpectralShape) – Spectral shape used for alignment.
interpolator (Optional[Type[colour.hints.TypeInterpolator]]) – Interpolator class type to use as interpolating function.
interpolator_kwargs (Optional[Dict]) – Arguments to use when instantiating the interpolating function.
extrapolator (Optional[Type[colour.hints.TypeExtrapolator]]) – Extrapolator class type to use as extrapolating function.
extrapolator_kwargs (Optional[Dict]) – Arguments to use when instantiating the extrapolating function.
- Returns
Aligned spectral distribution.
- Return type
Examples
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> sd = SpectralDistribution(data) >>> with numpy_print_options(suppress=True): ... print(sd.align(SpectralShape(505, 565, 1))) ... [[ 505. 0.0663929...] [ 506. 0.0666509...] [ 507. 0.0669069...] [ 508. 0.0671613...] [ 509. 0.0674150...] [ 510. 0.0676692...] [ 511. 0.0679253...] [ 512. 0.0681848...] [ 513. 0.0684491...] [ 514. 0.0687197...] [ 515. 0.0689975...] [ 516. 0.0692832...] [ 517. 0.0695771...] [ 518. 0.0698787...] [ 519. 0.0701870...] [ 520. 0.0705 ...] [ 521. 0.0708155...] [ 522. 0.0711336...] [ 523. 0.0714547...] [ 524. 0.0717789...] [ 525. 0.0721063...] [ 526. 0.0724367...] [ 527. 0.0727698...] [ 528. 0.0731051...] [ 529. 0.0734423...] [ 530. 0.0737808...] [ 531. 0.0741203...] [ 532. 0.0744603...] [ 533. 0.0748006...] [ 534. 0.0751409...] [ 535. 0.0754813...] [ 536. 0.0758220...] [ 537. 0.0761633...] [ 538. 0.0765060...] [ 539. 0.0768511...] [ 540. 0.0772 ...] [ 541. 0.0775527...] [ 542. 0.0779042...] [ 543. 0.0782507...] [ 544. 0.0785908...] [ 545. 0.0789255...] [ 546. 0.0792576...] [ 547. 0.0795917...] [ 548. 0.0799334...] [ 549. 0.0802895...] [ 550. 0.0806671...] [ 551. 0.0810740...] [ 552. 0.0815176...] [ 553. 0.0820049...] [ 554. 0.0825423...] [ 555. 0.0831351...] [ 556. 0.0837873...] [ 557. 0.0845010...] [ 558. 0.0852763...] [ 559. 0.0861110...] [ 560. 0.087 ...] [ 561. 0.0879383...] [ 562. 0.0889300...] [ 563. 0.0899793...] [ 564. 0.0910876...] [ 565. 0.0922541...]]
- trim(shape: colour.colorimetry.spectrum.SpectralShape) colour.colorimetry.spectrum.SpectralDistribution [source]¶
Trim the spectral distribution wavelengths to given spectral shape.
- Parameters
shape (colour.colorimetry.spectrum.SpectralShape) – Spectral shape used for trimming.
- Returns
Trimmed spectral distribution.
- Return type
Examples
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> sd = SpectralDistribution(data) >>> sd = sd.interpolate(SpectralShape(500, 600, 1)) >>> with numpy_print_options(suppress=True): ... print(sd.trim(SpectralShape(520, 580, 5))) ... [[ 520. 0.0705 ...] [ 521. 0.0708155...] [ 522. 0.0711336...] [ 523. 0.0714547...] [ 524. 0.0717789...] [ 525. 0.0721063...] [ 526. 0.0724367...] [ 527. 0.0727698...] [ 528. 0.0731051...] [ 529. 0.0734423...] [ 530. 0.0737808...] [ 531. 0.0741203...] [ 532. 0.0744603...] [ 533. 0.0748006...] [ 534. 0.0751409...] [ 535. 0.0754813...] [ 536. 0.0758220...] [ 537. 0.0761633...] [ 538. 0.0765060...] [ 539. 0.0768511...] [ 540. 0.0772 ...] [ 541. 0.0775527...] [ 542. 0.0779042...] [ 543. 0.0782507...] [ 544. 0.0785908...] [ 545. 0.0789255...] [ 546. 0.0792576...] [ 547. 0.0795917...] [ 548. 0.0799334...] [ 549. 0.0802895...] [ 550. 0.0806671...] [ 551. 0.0810740...] [ 552. 0.0815176...] [ 553. 0.0820049...] [ 554. 0.0825423...] [ 555. 0.0831351...] [ 556. 0.0837873...] [ 557. 0.0845010...] [ 558. 0.0852763...] [ 559. 0.0861110...] [ 560. 0.087 ...] [ 561. 0.0879383...] [ 562. 0.0889300...] [ 563. 0.0899793...] [ 564. 0.0910876...] [ 565. 0.0922541...] [ 566. 0.0934760...] [ 567. 0.0947487...] [ 568. 0.0960663...] [ 569. 0.0974220...] [ 570. 0.0988081...] [ 571. 0.1002166...] [ 572. 0.1016394...] [ 573. 0.1030687...] [ 574. 0.1044972...] [ 575. 0.1059186...] [ 576. 0.1073277...] [ 577. 0.1087210...] [ 578. 0.1100968...] [ 579. 0.1114554...] [ 580. 0.1128 ...]]
- normalise(factor: Number = 1) colour.colorimetry.spectrum.SpectralDistribution [source]¶
Normalise the spectral distribution using given normalization factor.
- Parameters
factor (Number) – Normalization factor.
- Returns
Normalised spectral distribution.
- Return type
Examples
>>> from colour.utilities import numpy_print_options >>> data = { ... 500: 0.0651, ... 520: 0.0705, ... 540: 0.0772, ... 560: 0.0870, ... 580: 0.1128, ... 600: 0.1360 ... } >>> sd = SpectralDistribution(data) >>> with numpy_print_options(suppress=True): ... print(sd.normalise()) [[ 500. 0.4786764...] [ 520. 0.5183823...] [ 540. 0.5676470...] [ 560. 0.6397058...] [ 580. 0.8294117...] [ 600. 1. ...]]