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template<typename T , CSpectralSampleProps SampleProps> |
constexpr T | ph::math::wavelength_interval_of () noexcept |
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template<typename T , CSpectralSampleProps SampleProps> |
constexpr auto | ph::math::wavelength_range_of (const std::size_t sampleIndex) noexcept -> std::pair< T, T > |
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
T | ph::math::estimate_samples_energy (const TSpectralSampleValues< T, SampleProps > &srcSamples) |
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::normalize_samples_energy (const TSpectralSampleValues< T, SampleProps > &srcSamples) |
| Normalize spectral samples as if they carry energy. Normalized spectral samples, together, represents the expected amount of energy that 1 unit of total energy would distribute on each wavelength interval (implying that the samples should sum to 1).
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
constexpr TSpectralSampleValues< T, SampleProps > | ph::math::constant_spectral_samples (T constant) |
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template<typename T , typename U , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_spectral_samples (const U *wavelengthsNM, const U *values, std::size_t numPoints, ESpectralResample algorithm=ESpectralResample::Default) |
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_black_body (T temperatureK) |
| SPD of black-body radiation, with total energy = 1.
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_black_body_radiance (T temperatureK) |
| SPD of black-body radiation in radiance. If a normalized energy distribution is desired, use resample_black_body() .
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_black_body_spectral_radiance (T temperatureK) |
| SPD of black-body radiation in spectral radiance. Note that this function is not returning radiance but spectral radiance. The returned spectral radiance has the unit of watt per steradian per square meter per meter (W * sr^-1 * m^-2 * m^-1). If radiance is desired, use resample_black_body_radiance() . If a normalized energy distribution is desired, use resample_black_body() .
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps, EReferenceWhite NORMALIZER = EReferenceWhite::D65> |
TTristimulusValues< T > | ph::math::spectral_samples_to_CIE_XYZ (const TSpectralSampleValues< T, SampleProps > &srcSamples, EColorUsage usage) |
| Converting spectral samples to CIE-XYZ using standard CMFs.
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_illuminant_E () |
| SPD of standard illuminants. Any light source which statistically has the same relative SPD as a standard illuminant can be considered a standard light source, and is the reason why the SPD resample functions return a energy-normalized SPD (for convenience, as this is what you want almost always).
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template<typename T , CSpectralSampleProps SampleProps = DefaultSpectralSampleProps> |
TSpectralSampleValues< T, SampleProps > | ph::math::resample_illuminant_D65 () |
| SPD of standard illuminants D65, with total energy = 1.
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