2021
DOI: 10.1038/s41598-021-02810-1
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Air temperature drives the evolution of mid-infrared optical properties of butterfly wings

Abstract: This study uncovers a correlation between the mid-infrared emissivity of butterfly wings and the average air temperature of their habitats across the world. Butterflies from cooler climates have a lower mid-infrared emissivity, which limits heat losses to surroundings, and butterflies from warmer climates have a higher mid-infrared emissivity, which enhances radiative cooling. The mid-infrared emissivity showed no correlation with other investigated climatic factors. Phylogenetic independent contrasts analysis… Show more

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Cited by 8 publications
(3 citation statements)
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“…This suggests that both hair density, as well as structural features of the hairs (S2 Fig), may contribute to the reflectance profile differences across male morphs and females. Microstructural features of insect hairs and scales are known to influence their reflective properties in both the NIR and mid-infrared [6,8,46]. The striations on the external surface of the hair (S2 Fig) are reminiscent of the hairs of the Saharan silver ant [8].…”
Section: Discussionmentioning
confidence: 99%
“…This suggests that both hair density, as well as structural features of the hairs (S2 Fig), may contribute to the reflectance profile differences across male morphs and females. Microstructural features of insect hairs and scales are known to influence their reflective properties in both the NIR and mid-infrared [6,8,46]. The striations on the external surface of the hair (S2 Fig) are reminiscent of the hairs of the Saharan silver ant [8].…”
Section: Discussionmentioning
confidence: 99%
“…As the temperature of an object increases, the object emits more thermal flux. The thermal flux is defined as total energy radiated per unit surface in time, and it is referred to by various names, including black-body irradiance, energy flux density, radiant flux, or emissive power [26][27][28] . According to Stefan-Boltzmann law, thermal flux (I) is a function of temperature (T) and a proportional constant (μ).…”
Section: Background Theorymentioning
confidence: 99%
“…The thermal ux is de ned as total energy radiated per unit surface in time, and it is referred to by various names, including blackbody irradiance, energy ux density, radiant ux, or emissive power (Stipetic et al 2011;Holland and Reusser. 2016; Krishna et al 2021). According to Stefan-Boltzmann law, thermal ux (I) is a function of temperature (T) and a proportional constant (µ).…”
Section: Background Theorymentioning
confidence: 99%