Adaptive Variable Emissivity Reflector for Seasonal and Daily Thermal Regulation in Regions with Significant Temperature Variations
Source abstract
Abstract
Abstract Temperature‐adaptive variable emissivity reflectors offer an electricity‐free and environmentally friendly cooling strategy, holding substantial potential to improve the global energy landscape. However, challenges associated with unoptimized solar absorptance can lead to overcooling or overheating when the modulation of infrared emittance is held constant, thereby increasing extra energy consumption. Herein, a temperature‐adaptive variable emissivity reflector based on W‐Mg co‐doped VO2 (W‐Mg‐VER) is proposed, engineered to optimize solar absorptance (αL = 0.40) while maintaining effective infrared emittance modulation (Δɛ = 0.69) near ambient temperature. To maximize year‐round energy savings in regions experiencing significant daily temperature fluctuations, W‐Mg co‐doped VO2 is employed to reduce solar absorptance by modifying electron occupancy in the V 3d orbital and expanding the optical bandgap. Outdoor experiments have validated the remarkable temperature management and energy‐saving capabilities of the W‐Mg‐VER, facilitated by its seamless transition between radiative cooling and heat‐retaining modes. Numerical simulation indicates that a W‐Mg‐VER roof covering 100 m2 would save 152.9 GJ of energy annually in locations with significant daily temperature variations. Moreover, W‐Mg‐VER demonstrates robust performance, exhibiting less than 1% degradation in emittance tunability and solar absorptance after 10 000 cycles. This approach provides valuable insights and practical guidance for significantly enhancing global energy savings.
Source: crossref · Quality: baseline
Research context
OpenAlex topics: Thermal Radiation and Cooling Technologies · Urban Heat Island Mitigation · Building Energy and Comfort Optimization
SciVX discovery tags are terminology-based. OpenAlex topics are source-provided classifications.
Affiliations
Center for Composite Material and Structure Harbin Institute of Technology Harbin 150001 P. R. China
Institute of Marine Optoelectronic Equipment Harbin Institute of Technology Weihai 264209 P. R. China
Henan Key Laboratory of Infrared Spectrum Measures and Applications School of Physics Henan Normal University Xinxiang Henan 453007 P. R. China
Suzhou Laboratory Suzhou 215123 P. R. China
Funding
National Natural Science Foundation of China
References (45)
Show source-provided references
1. 10.1002/adfm.20190756210.1002/adfm.201907562 ↗
2. 10.1126/science.aat951310.1126/science.aat9513 ↗
3. 10.1021/acsphotonics.6b0099110.1021/acsphotonics.6b00991 ↗
4. 10.1002/adfm.20220358210.1002/adfm.202203582 ↗
5. 10.1002/adfm.20180218010.1002/adfm.201802180 ↗
6. 10.1038/s41467-019-09589-w10.1038/s41467-019-09589-w ↗
7. 10.1039/D3EE04261H10.1039/D3EE04261H ↗
8. 10.1002/smll.20210044610.1002/smll.202100446 ↗
9. 10.1002/adma.20200069710.1002/adma.202000697 ↗
10. 10.1021/acsami.1c2340110.1021/acsami.1c23401 ↗
11. 10.1126/science.abf713610.1126/science.abf7136 ↗
12. 10.1021/acsami.1c1791410.1021/acsami.1c17914 ↗
13. 10.1016/j.joule.2023.09.01110.1016/j.joule.2023.09.011 ↗
14. 10.1016/j.solmat.2011.08.01410.1016/j.solmat.2011.08.014 ↗
15. 10.1016/j.solmat.2013.07.02310.1016/j.solmat.2013.07.023 ↗
16. 10.1063/1.479227710.1063/1.4792277 ↗
17. 10.1038/s41598-019-47572-z10.1038/s41598-019-47572-z ↗
18. 10.1002/adfm.20230735610.1002/adfm.202307356 ↗
19. 10.1063/1.489361610.1063/1.4893616 ↗
20. 10.1021/nl400428310.1021/nl4004283 ↗
21. 10.1016/j.apsusc.2015.03.11610.1016/j.apsusc.2015.03.116 ↗
22. 10.1016/j.applthermaleng.2023.12175110.1016/j.applthermaleng.2023.121751 ↗
23. 10.1364/OE.26.00A77710.1364/OE.26.00A777 ↗
24. 10.1126/science.aaf547110.1126/science.aaf5471 ↗
25. 10.1016/j.solener.2020.08.07710.1016/j.solener.2020.08.077 ↗
26. 10.1063/5.008434110.1063/5.0084341 ↗
27. 10.1016/j.jallcom.2021.16267910.1016/j.jallcom.2021.162679 ↗
28. 10.1016/j.solmat.2019.11026010.1016/j.solmat.2019.110260 ↗
29. 10.1016/j.joule.2018.06.01810.1016/j.joule.2018.06.018 ↗
30. 10.1039/D0TC03436C10.1039/D0TC03436C ↗
31. 10.1063/1.476616710.1063/1.4766167 ↗
32. 10.1016/j.ssc.2022.11471010.1016/j.ssc.2022.114710 ↗
33. 10.1039/c3cp52009a10.1039/c3cp52009a ↗
34. 10.1016/j.apmt.2020.10080810.1016/j.apmt.2020.100808 ↗
35. 10.1021/acsami.3c1728610.1021/acsami.3c17286 ↗
36. 10.1016/j.apsusc.2014.03.07710.1016/j.apsusc.2014.03.077 ↗
37. 10.1038/s41467-021-24527-510.1038/s41467-021-24527-5 ↗
38. 10.1016/j.apsusc.2021.15199010.1016/j.apsusc.2021.151990 ↗
39. 10.1016/j.cej.2023.14209510.1016/j.cej.2023.142095 ↗
40. 10.1002/adfm.20231531510.1002/adfm.202315315 ↗
41. 10.1016/j.rser.2014.08.03910.1016/j.rser.2014.08.039 ↗
42. 10.1039/C7TC05536F10.1039/C7TC05536F ↗
43. 10.1016/j.ceramint.2020.02.14710.1016/j.ceramint.2020.02.147 ↗
44. 10.1103/PhysRevB.59.175810.1103/PhysRevB.59.1758 ↗
45. 10.1103/PhysRevB.57.150510.1103/PhysRevB.57.1505 ↗