Class SpectralAnalysis
java.lang.Object
org.episteme.natural.physics.classical.spectroscopy.SpectralAnalysis
Blackbody radiation and spectral analysis.
- Since:
- 1.0
- Author:
- Silvere Martin-Michiellot, Gemini AI (Google DeepMind)
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Field Summary
Fields -
Method Summary
Modifier and TypeMethodDescriptionstatic RealcolorTemperature(Real peakWavelengthMeters) Color temperature from peak wavelengthstatic RealphotonEnergy(Real wavelengthMeters) Photon energy: E = hc/λstatic RealplanckRadiance(Real wavelengthMeters, Real temperatureKelvin) Planck radiance: B(λ,T) = (2hc²/λâµ) / (exp(hc/λkT) - 1)static RealstefanBoltzmannPower(Real areaM2, Real temperatureKelvin) Stefan-Boltzmann: P = ÃÂÆ’ * A * Tâ´static RealwavelengthFromEnergy(Real energyJoules) Wavelength from energy: λ = hc/Estatic RealwienPeakWavelength(Real temperatureKelvin) Wien's displacement law: λ_max = b / T
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Field Details
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H
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C
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K
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WIEN_B
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SIGMA
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Method Details
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wienPeakWavelength
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stefanBoltzmannPower
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planckRadiance
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photonEnergy
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wavelengthFromEnergy
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colorTemperature
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