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Objects typically betray their presence through two types of signals: reflected signals from external light sources and thermal emission signals from the objects themselves (Fig 1a). On the one hand, objects in nature are illuminated by external light sources, among which solar radiance is the most significant. Solar radiance emits its energy mainly in the spectral range of 0.15–4 μm and plays a crucial role in the visible (VIS, 400–780 nm), near-infrared (NIR, 0.78–1.4 μm), and short-wave infrared (SWIR, 1.4–2.5 μm) detection bands. On the other hand, objects radiate energy through thermal emission, which can be detected by detectors that work in atmospheric transmission windows (mid-wave infrared (MWIR, 3–5 μm) and long-wave infrared (LWIR, 8–14 μm)). With temperature rising, the peak wavelength of thermal emission shifts to the short-wave direction, making the radiative signal in the SWIR band non-negligible.
In a new paper (doi: 10.1038/s41377-023-01287-z ) published in Light Science & Application, a team of scientists, led by Professor Qiang Li from State Key Laboratory of Modern Optical Instrumentation, College of Optical Science and Engineering, Zhejiang University, China, and co-workers have developed a whole-infrared-band camouflage device, which is compatible with radiative heat dissipation in two undetected bands (2.5–3 μm and 5–8 μm). Based on the understanding of the signal sources, they proposed the spectral features of camouflage devices (Fig 1b):
- In the SWIR band, low emissivity has a wider scope of application. The highest irradiance of sunshine is similar to that of a 330 °C blackbody. However, in practical scenarios, where solar irradiance is generally lower than its highest level, inhibiting thermal emission makes greater contributions to reducing total signal intensity.
- In the MWIR and LWIR bands, low emissivity is more suitable as thermal emission usually dominates the detected signal and the intensity of sunshine is weak enough to be negligible.
- In the VIS and NIR bands, low reflectivity is preferable since the predominant source of detected signal is reflected solar radiance and thermal emission is generally insignificant.
The Al2O3/Ge/Al2O3/Ge/ZnS/GST/Ni multilayer structure is employed to modulate the ultra-broad spectrum from the visible to the LWIR range (Fig 2a). The unique architecture of this structure allows it to cater to the varying demands of the entire infrared range and the visible range, while concurrently achieving efficient radiative heat dissipation within two undetected bands (Fig 2a).
Appearing gray-blue, the fabricated sample exhibits low average reflectivity in the VIS/NIR bands (0.129/0.281) (Fig 2b). When heating up to 200 °C, the radiative (apparent) temperatures of the sample under the MWIR/LWIR cameras are merely 86.3 ℃/94.7 ℃ (Fig 2c). Compared to the reference blackbody, the signal intensity of the sample is 39.3% lower under the SWIR camera (Fig 2c). Particularly, the SWIR camouflage performance is demonstrated under solar radiance. At higher temperatures, the sample exhibits smaller signal intensity than the Cr reference in all observing directions. While at lower temperatures, the sample maintains the edge except in the specular reflection direction of solar radiance.
The efficacy of radiative heat dissipation is demonstrated by putting the sample and the Cr reference subjected to the same input electrical heating power. At 20 W input power
(equivalent to a power density of 2000 Wm−2), the surface temperature of the sample is 174.5 °C, which is 14.4 °C lower than that of the Cr reference.
These lower surface temperatures help to reduce thermal load and improve the performance of MWIR and LWIR camouflage.
“This work provides a comprehensive guideline for developing camouflage technologies compatible with radiative heat dissipation, against complicated signal sources and multispectral detective technologies.” the scientists noted.
“This device for whole-infrared-band camouflage can facilitate applications that require sophisticated spectrum manipulation and stimulate innovative avenues for modern thermal management technologies and contribute to an energy-efficient future.” they forecast.
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References
DOI
Original Source URL
https://doi.org/10.1038/s41377-023-01287-z
Funding information
This work was supported by the National Natural Science Foundation of China (Grant No. 61975181).
About Light: Science & Applications
The Light: Science & Applications will primarily publish new research results in cutting-edge and emerging topics in optics and photonics, as well as covering traditional topics in optical engineering. The journal will publish original articles and reviews that are of high quality, high interest and far-reaching consequence.
