Geometrical-based quasi-aspheric surface description and design method for miniature, low-distortion, wide-angle camera lens

2020 ◽  
Vol 59 (27) ◽  
pp. 8408
Author(s):  
Zhenfeng Zhuang ◽  
Xavier Dallaire ◽  
Jocelyn Parent ◽  
Patrice Roulet ◽  
Simon Thibault
2020 ◽  
Vol 17 (03) ◽  
pp. 2050010
Author(s):  
Saeed Saeedvand ◽  
Hadi S. Aghdasi ◽  
Jacky Baltes

Although there are several popular and capable humanoid robot designs available in the kid-size range, they lack some important characteristics: affordability, being user-friendly, using a wide-angle camera, sufficient computational resources for advanced AI algorithms, and mechanical robustness and stability are the most important ones. Recent advances in 3D printer technology enables researchers to move from model to physical implementation relatively easy. Therefore, we introduce a novel fully 3D printed open platform humanoid robot design named ARC. In this paper, we discuss the mechanical structure and software architecture. We show the capabilities of the ARC design in a series of experimental evaluations.


2012 ◽  
Author(s):  
Vania Da Deppo ◽  
Fiorangela La Forgia ◽  
Giampiero Naletto ◽  
Maria-Guglielmina Pelizzo ◽  
Cesare Barbieri

2018 ◽  
Vol 33 (1) ◽  
pp. 199-205 ◽  
Author(s):  
Yusuke Sumi ◽  
Hiroyuki Egi ◽  
Minoru Hattori ◽  
Takahisa Suzuki ◽  
Masakazu Tokunaga ◽  
...  

2013 ◽  
Vol 42 (4) ◽  
pp. 456-461
Author(s):  
薛庆生 XUE Qing-sheng ◽  
王淑荣 WANG Shu-rong ◽  
陈伟 CHEN Wei
Keyword(s):  

2020 ◽  
Vol 12 (22) ◽  
pp. 3676
Author(s):  
Xuesen Xu ◽  
Jianjun Liu ◽  
Dawei Liu ◽  
Bin Liu ◽  
Rong Shu

The main objective of this study is to develop a Hapke photometric model that is suited for Chang’E-1 (CE-1) Interference Imaging Spectrometer (IIM) data. We first divided the moon into three areas including ‘maria’, ‘new highland’ and old ‘highland’ with similar photometry characteristic based on the Hapke parameters of the moon derived from Lunar Reconnaissance Orbiter Camera (LROC) Wide Angle Camera (WAC) multispectral data. Then, we selected the sample data in the ‘maria’ area and obtained a new set of Hapke model’s parameters that can best fit these data. Result shows that photometric correction using Hapke model with these new derived parameters can eliminate the effect of variations in viewing and luminating geometry, especially ‘opposition surge’, more efficiently than the empirical model. The corrected mosaic shows no significant artifacts along the tile boundaries and more detailed information of the image can be exhibited due to a better correction of ‘opposition surge’ at small phase angle (g < 15°).


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