ultraviolet reflectance
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Author(s):  
María Victoria de Gálvez ◽  
José Aguilera ◽  
María Leal ◽  
Cristina Sánchez‐Roldán ◽  
Enrique Herrera‐Ceballos

2021 ◽  
Vol 2 (5) ◽  
pp. 189
Author(s):  
Benjamin D. Byron ◽  
Kurt D. Retherford ◽  
Elizabeth Czajka ◽  
Joshua T. S. Cahill ◽  
Amanda R. Hendrix ◽  
...  

2021 ◽  
Vol 109 (3) ◽  
Author(s):  
Jacob F. Penner ◽  
Maria A. Eifler ◽  
Douglas A. Eifler

Author(s):  
Justin Yeager ◽  
James Barnett

Warning signals are often characterized by highly contrasting, distinctive and memorable colors. Both chromatic (hue) and achromatic (brightness) contrast contribute to signal efficacy, making longwave colored signals (red and yellow) that generate both chromatic and achromatic contrast common. Shortwave colors (blue and ultraviolet) do not contribute to luminance perception, yet are also common in warning signals. The presence of UV aposematic signals is paradoxical as UV perception is not universal, and evidence for its utility is at best mixed. We used visual modeling to quantify how UV affects signal contrast in aposematic butterflies and frogs. We found that UV only appreciably affected visual contrast in the butterflies. As the butterflies, but not the frogs, have UV-sensitive vision these results support the notion that UV reflectance is associated with intraspecific communication, but appears to be non-functional in frogs. Consequently, we should be careful when assigning a selection-based benefit from UV reflectance.


2021 ◽  
Vol 258 ◽  
pp. 112404
Author(s):  
Huizeng Liu ◽  
Xianqiang He ◽  
Qingquan Li ◽  
Susanne Kratzer ◽  
Junjie Wang ◽  
...  

OSA Continuum ◽  
2021 ◽  
Author(s):  
Yuka Esashi ◽  
Michael Tanksalvala ◽  
Zhe Zhang ◽  
Nicholas Jenkins ◽  
Henry Kapteyn ◽  
...  

Author(s):  
Giuseppe Scardera ◽  
David Payne ◽  
Muhammad Umair Khan ◽  
Yu Zhang ◽  
Anastasia Soeriyadi ◽  
...  

2021 ◽  
Vol 7 (4) ◽  
pp. eaba5749
Author(s):  
Mark Elowitz ◽  
Bhalamurugan Sivaraman ◽  
Amanda Hendrix ◽  
Jen-Iu Lo ◽  
Sheng-Lung Chou ◽  
...  

We present the first analysis of far-ultraviolet reflectance spectra of regions on Rhea’s leading and trailing hemispheres collected by the Cassini Ultraviolet Imaging Spectrograph during targeted flybys. In particular, we aim to explain the unidentified broad absorption feature centred near 184 nm. We have used laboratory measurements of the UV spectroscopy of a set of candidate molecules and found a good fit to Rhea’s spectra with both hydrazine monohydrate and several chlorine-containing molecules. Given the radiation-dominated chemistry on the surface of icy satellites embedded within their planets’ magnetospheres, hydrazine monohydrate is argued to be the most plausible candidate for explaining the absorption feature at 184 nm. Hydrazine was also used as a propellant in Cassini’s thrusters, but the thrusters were not used during icy satellite flybys and thus the signal is believed to not arise from spacecraft fuel. We discuss how hydrazine monohydrate may be chemically produced on icy surfaces.


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