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Updated: Feb 10, 2026

Simulation, Fabrication and Characterization of THz Metamaterial Absorbers
Published on: December 27, 2012
Characterization of selective solar absorber under high vacuum
Researchers measured solar absorber properties under vacuum, reaching over 300°C. This data helps predict the performance of evacuated solar panels in real-world operating conditions.
Area of Science:
- Materials Science
- Renewable Energy Engineering
- Thermodynamics
Background:
- Selective solar absorbers are crucial for efficient solar thermal energy conversion.
- Understanding optical properties (absorption and emission) at elevated temperatures is vital for performance prediction.
- High vacuum conditions minimize convective heat losses, allowing accurate measurement of intrinsic material properties.
Purpose of the Study:
- To measure the total absorption and emission coefficients of selective solar absorbers.
- To determine these coefficients from room temperature up to stagnation temperature under high vacuum.
- To evaluate the solar absorptance and thermal emittance at various temperatures for performance modeling.
Main Methods:
- Selective solar absorbers were tested under high vacuum conditions (pressure not specified).
- Samples were illuminated with a solar simulator at 1000W/m².
- Sample temperature was monitored during heating, equilibrium, and cooling phases to determine stagnation temperature.
- Data analysis was performed to derive absorption and emission coefficients.
Main Results:
- The absorber reached a stagnation temperature exceeding 300°C without solar concentration.
- Solar absorptance and thermal emittance were evaluated at different temperatures.
- The measured coefficients provide insights into the absorber's behavior at operating conditions.
Conclusions:
- The study successfully characterized the optical properties of selective solar absorbers under vacuum and elevated temperatures.
- The obtained data is essential for accurate performance prediction of evacuated solar collectors.
- This research contributes to the development of more efficient solar thermal energy systems.
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