Liyan Wua,
Wentao Rena,
Yuqiu Songa,
Mingjin Xina,
Shichao Niub and
Zhiwu Han*b
aCollege of Engineering, Shenyang Agricultural University, Shenyang, 110866, P. R. China
bKey Laboratory of Bionic Engineering (Ministry of Education, China), Jilin University, Changchun 130022, P. R. China. E-mail: zwhan@jlu.edu.cn
First published on 28th April 2015
When the sunlight irradiates the surface of butterfly wings, it can be absorbed by the microstructures in the wings scales and converted into heat to maintain the butterfly’s metabolism. This phenomenon is an inspiration which is facilitating the scientific research in solar energy utilization. In this study, the absorption characteristics of seven species of butterfly were investigated using a spectrometer. It was found that the butterfly Heliophorus ila Lvcaenidae showed more efficient absorption capability (absorptivity was about at 85%) compared with other species in the wavelength range from 230 nm to 850 nm. Then, the morphology and structures of the butterfly Heliophorus ila Lvcaenidae wing scales were examined by Scanning Electron Microscope (SEM) and Transmission Electron Microscope (TEM). The results showed that there were two kinds of scales distributed on the wing surface of the butterfly Heliophorus ila Lvcaenidae. Finally, the optical mechanisms were revealed by theories of multiple reflection and resonance. It was confirmed that the hierarchical hollow nano-architectures of the scales were responsible for the high-efficiency absorption behaviour. This study could be used as a theoretical reference for subsequent bionic design of structural materials for solar energy utilization.
Recent studies showed that there were certain species appearing in very early spring (April or May) at high altitude mountainous areas, where energy was used to protect their body from cold climate, which depended on the efficient sunlight absorption of their wing surface scales (Fig. 1). In addition, during the breeding season, more energy was needed to gestate eggs, while the energy could not be provided by their body due to the decline of its mobility. Therefore, more solar energy should be obtained for energy demand during this period. The efficient absorption relied on not only the arrangement format, but also mainly the delicate nano-architecture inner scales.
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Fig. 1 Image of butterfly Heliophorus ila Lvcaenidae and distribution of the scales on its wing surface. |
In this work, a spectrometer was employed to test optical characteristics of 7 kinds of butterflies. The results illustrated that the butterfly Heliophorus ila Lvcaenidae scales had the best sunlight absorbing effect with absorptivity reaching up to 85%. The microstructures of butterfly Heliophorus ila Lvcaenidae scales were studied with SEM and TEM and simplified models were then built up. The cross section image of butterfly Heliophorus ila Lvcaenidae scales had two hierarchies of microstructures. The upper part had a hollow trianglar form that resulted in multiple reflections and refractions. The bottom hollow layer formed a rectangular resonant cavity model which had light trapping effect. The solar energy was absorbed efficiently due to the integrated function of these two mechanisms. This study demonstrated an enlightening way to exploit bionic designing of structural materials for solar heat utilization.
Test specimens were taken from single pure color areas of abdomen wings and with complete scales to avoid influence on the optical measurements by any eyespot or other colors. Tests were carried out under the same conditions: trial wavelength range within 230–800 nm with 0° incident angle. Reference light with an incident angle of 8°. The temperature of the laboratory was at 15–30 °C. Relative humidity was less than 65%. Finally, the absorption curves were obtained and the scales with best absorption effect were selected to be examined further.
Three optical effects may occur when light reaches the wing surface, namely, reflection, transmission and absorption. The sum of the three portions of light should be 100% as shown in eqn (1). When the transmission was at a certain level, a lower reflectivity means a higher absorptivity. The absorption capacity could be evaluated by calculating the absorptivity based on the formula.
Reflectivity (R%) + Absorbtivity (A%) + Transmissivity (T%) = 100% | (1) |
For clear comparison, the curves were displayed in Fig. 2a and b separately. In the full trial spectrum, Papilio maackii shining area and Apatura ilia exhibited higher reflectance, shown as Fig. 2-I and V. This meant their absorptivities were lower. Furthermore, these two curves demonstrated steady tendency and had not any peak value within the whole spectrum. Reflectivity of Papilio machaon, Parnassius stubbendorfii, Brenthis daphne, Troides brookiana increased with wavelength obviously, shown as Fig. 2-II, III, VI and VII. The reflectivity value reached its highest point in the red spectrum. Butterfly Heliophorus ila Lvcaenidae (Fig. 2-IV) had the lowest reflectivity among all the samples. The minimal value plunged to 15%. It meant the absorptivity of butterfly Heliophorus ila Lvcaenidae could be as much as 85%. Furthermore, its absorptivity almost remained at a constant level within the entire trial spectrum without any obvious peak.
The reflectivity of the black area of butterfly Papilio maackii (Fig. 2-VIII) reached 50%, which was higher than that of butterfly Heliophorus ila Lvcaenidae and a spectral peak emerged at 650 nm. After the primary optical testes and analysis, butterfly Heliophorus ila Lvcaenidae scales were selected to be further observed at a micro level with SEM and TEM.
More micro details of a single scale were obtained at higher magnification. Shown in Fig. 3b, there were parallel ridges distributing from front to end on every scale. There were also many short ribs (the length varied at 100–200 μm) connecting each two adjacent ridges. The distances between each two ribs were almost same, and therefore some rectangular lattices were formed which looked like thousands of windows. The regular through-holes structures of the cover scales (type 1 scales) in this manuscript could scatter the incident light, resulting in more and more incident light irradiating on the surface of the ground scales (type 2 scales). Finally, most of the light energy could be absorbed by the ground scales. The role of the cover scales (type 1 scales) was mainly diffracting light. So, they were largely conducive to absorption instead of direct absorption. There were other kinds of disordered nano-hole structure like this were also found in other butterflies.29,30
Details of type 2 scales also had ridges (Fig. 3c). However, the difference was that the ridges were more densely distributed and had a greater width. Spacing between two ridges was about 0.5–0.8 μm. Therefore, ridges occupied a larger proportion of the lit area and played a main role in sunlight absorption.
Therefore, even though there were two kinds of scales on butterfly Heliophorus ila Lvcaenidae wings, the upper scales had a holes structure and rarely absorb sunlight. The underlying scales with ridges have absorption capability.
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Fig. 4 Microstructure model of scales with absorption function. (a) TEM image of scale microstructure. (b) 3D simplified model. |
n1![]() ![]() ![]() ![]() | (2) |
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Fig. 5 Schematic of the multiple reflection and refraction occurred on the upper part of the structures of the scale surface. |
In this case, n2 > n1. So, γ < α. The refraction light travelled across the materials and entered into the hollow zone. Then, refraction and reflection occurred at any interface. After multiple reflections and refractions, light travelled for a longer distance, and only a small part of light was reflected back to the air, resulting in most of the incident light being effectively adsorbed within the structure eventually.
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Fig. 6 Schematic of the light absorption occurred on the bottom part of the structures of the scale surface. |
In this case, the bottom part of the scales could be optimized as a rectangular cavity of six planes as shown in Fig. 6. The coordinates of the inner surface are shown as eqn (3).
![]() | (3) |
The electric field of the electromagnetic wave inside the cavity is E and magnetic field is H. Any rectangular components of E and H should meet the Helmholtz equation. For any component of u(x,y,z), there was ∇2u + k2u = 0,33 based on separation of variables method. If it is supposed that u(x,y,z) = X(x)Y(y)Z(z), then
![]() | (4) |
kx2 + ky2 + kz2 = ω2με | (5) |
So, the result of u(x,y,z) was
u(x,y,z,) = (C1![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() | (6) |
Established boundary conditions were n⇀ × E⇀ = 0,∂En/∂n = 0 and x = 0, y = 0, z = 0. The arbitrary constant Ci and Di can be defined, and as a result u(x,y,z) can be specified as a component of E⇀.
![]() | (7) |
In terms of boundary conditions on planes of x = L1, y = L2, z = L3, it is true that kxL1, kyL2, kzL3 must be an integer times π, namely
![]() | (8) |
In eqn (8), m, n, p represent numbers of half-wave contained in each rectangle side.
After substituting eqn (7) into ∇ = 0, the three arbitrary constants A1, A2, A3 must fit the relation shown in eqn (9).
kxA1 + kyA2 + kzA3 = 0 | (9) |
It can be concluded from eqn (9) that two out of the constants A1, A2, A3 were independent. After satisfying eqn (8) and (9), eqn (7) could be considered as one sort of region oscillation of the electromagnetic field inside the rectangular hollow structure.
For each group of m, n, p, there are two independent polarized wave modes, and the resonant frequency ω can be obtained from eqn (5) and (10).
![]() | (10) |
![]() | (11) |
Above was the ideal mode of resonant cavity. In this study, of the butterfly Heliophorus ila Lvcaenidae, the scale material consisted of a rectangular cavity. L1 = 580 nm, L2 = 130 nm, L3 ≫ L1, L2, the materials had a certain energy consumption. The light wave bounced back and forth on the cavity wall. In this process, a portion of light was consumed and absorbed by the materials. Certain light with wavelength λ110 was strengthened and reflected back to the air from certain flaws position and produced the wings structural color of butterfly Heliophorus ila Lvcaenidae. In this case, the calculation result was λ110 = 253.7 nm, that is why there was an non-obvious peak nearby 250 nm spectrum region of curve-IV in Fig. 2a.
SEM results showed that butterfly Heliophorus ila Lvcaenidae had two kinds of scales. Sunlight passed through the holes in the scales on the surface and irradiated on the underlying scales. The underlying scales played a main role in the absorbing behavior.
TEM analysis illustrated the cross section microstructure of scales type 2. There were two parts of optical delicate nano-architectures. The top part was simplified to a hollow triangle model. Sunlight was repeatedly reflected and refracted on the slope surface. In this way, the light travelled a longer path length in the scale materials. Therefore, more energy was consumed. The bottom part was simplified to a rectanglar resonator model. Incident light was reflected back and forth repeatedly. Energy was absorbed gradually and saved during this endless reflecting process. Only light with wavelength λ110 = 250 nm could be reflected out to show the structural color of butterfly Heliophorus ila Lvcaenidae.
This study focuses on the absorption mechanisms for the inner microstructures of the scales. The contents of this paper have an important reference value for solar heat utilization research via bionic design.
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