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Internal temperature inversion in semi-transparent materials based on spectral radiative transfer modeling.
Optics Express
|December 19, 2025
Summary
This study introduces a spectral inversion model for non-contact temperature measurement in challenging semi-transparent materials. The novel method accurately maps internal temperature distributions, even with noise, outperforming traditional infrared thermometry.
Area of Science:
- Physics
- Materials Science
- Thermodynamics
Background:
- Non-contact temperature measurement in semi-transparent materials is difficult due to optical properties and thermal gradients.
- Conventional infrared thermometry struggles with complex media, limiting thermal profiling accuracy.
Purpose of the Study:
- To develop an advanced spectral inversion model for precise non-contact temperature measurement in semi-transparent multilayer materials.
- To overcome limitations posed by optical inhomogeneities and depth-dependent thermal gradients.
Main Methods:
- Utilized a spectral inversion model based on the scattering matrix and fluctuation-dissipation theorem.
- Integrated simulated annealing algorithm with local ensemble averaging for high-precision temperature reconstruction.
- Validated the model through numerical simulations on five-layer thin-film structures with varying optical constants.
Main Results:
- Achieved high-precision reconstruction of internal temperature distribution in multilayer materials.
- Demonstrated robust performance under multiplicative uniform noise (0.5%-5%), with max relative errors below 0.67% at 5% noise.
- Successfully reconstructed temperature distributions in complex thin-film structures.
Conclusions:
- The proposed spectral inversion framework provides an accurate non-contact method for thermal profiling in challenging semi-transparent materials.
- This approach is suitable for complex media where conventional infrared thermometry is insufficient.
- Offers a significant advancement in non-contact thermal metrology for materials science and engineering.
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